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1 #LyX 2.1 created this file. For more info see http://www.lyx.org/
2 \lyxformat 474
3 \begin_document
4 \begin_header
5 \textclass aastex
6 \begin_preamble
7 \newcommand{\vdag}{(v)^\dagger}
8 \newcommand{\myemail}{skywalker@galaxy.far.far.away}
9 \slugcomment{Not to appear in Nonlearned J., 45.}
10 \shorttitle{Djorgovski et al.}
11 \shortauthors{Collapsed Cores in Globular Clusters}
12 \end_preamble
13 \use_default_options false
14 \maintain_unincluded_children false
15 \language english
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55 \suppress_date false
56 \justification true
57 \use_refstyle 0
58 \index Index
59 \shortcut idx
60 \color #008000
61 \end_index
62 \secnumdepth 3
63 \tocdepth 3
64 \paragraph_separation indent
65 \paragraph_indentation default
66 \quotes_language english
67 \papercolumns 1
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74 \html_be_strict false
75 \end_header
76
77 \begin_body
78
79 \begin_layout Title
80 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
81  Examples
82 \end_layout
83
84 \begin_layout Author
85 S.
86  Djorgovski
87 \begin_inset Flex altaffilmark
88 status open
89
90 \begin_layout Plain Layout
91 1,2,3
92 \end_layout
93
94 \end_inset
95
96  and Ivan R.
97  King
98 \begin_inset Flex altaffilmark
99 status collapsed
100
101 \begin_layout Plain Layout
102 1
103 \end_layout
104
105 \end_inset
106
107
108 \end_layout
109
110 \begin_layout Affiliation
111 Astronomy Department, University of California, Berkeley, CA 94720
112 \end_layout
113
114 \begin_layout Author
115 C.
116  D.
117  Biemesderfer
118 \begin_inset Flex altaffilmark
119 status collapsed
120
121 \begin_layout Plain Layout
122 4,5
123 \end_layout
124
125 \end_inset
126
127
128 \end_layout
129
130 \begin_layout Affiliation
131 National Optical Astronomy Observatories, Tucson, AZ 85719
132 \end_layout
133
134 \begin_layout Email
135 aastex-help@aas.org
136 \end_layout
137
138 \begin_layout And
139
140 \end_layout
141
142 \begin_layout Author
143 R.
144  J.
145  Hanisch
146 \begin_inset Flex altaffilmark
147 status collapsed
148
149 \begin_layout Plain Layout
150 5
151 \end_layout
152
153 \end_inset
154
155
156 \end_layout
157
158 \begin_layout Affiliation
159 Space Telescope Science Institute, Baltimore, MD 21218
160 \end_layout
161
162 \begin_layout Altaffilation
163 \begin_inset Argument 1
164 status open
165
166 \begin_layout Plain Layout
167 1
168 \end_layout
169
170 \end_inset
171
172 Visiting Astronomer, Cerro Tololo Inter-American Observatory.
173  CTIO is operated by AURA, Inc.
174 \begin_inset space \space{}
175 \end_inset
176
177 under contract to the National Science Foundation.
178 \end_layout
179
180 \begin_layout Altaffilation
181 \begin_inset Argument 1
182 status open
183
184 \begin_layout Plain Layout
185 2
186 \end_layout
187
188 \end_inset
189
190 Society of Fellows, Harvard University.
191 \end_layout
192
193 \begin_layout Altaffilation
194 \begin_inset Argument 1
195 status open
196
197 \begin_layout Plain Layout
198 3
199 \end_layout
200
201 \end_inset
202
203 present address: Center for Astrophysics, 60 Garden Street, Cambridge, MA
204  02138
205 \end_layout
206
207 \begin_layout Altaffilation
208 \begin_inset Argument 1
209 status open
210
211 \begin_layout Plain Layout
212 4
213 \end_layout
214
215 \end_inset
216
217 Visiting Programmer, Space Telescope Science Institute
218 \end_layout
219
220 \begin_layout Altaffilation
221 \begin_inset Argument 1
222 status open
223
224 \begin_layout Plain Layout
225 5
226 \end_layout
227
228 \end_inset
229
230 Patron, Alonso's Bar and Grill
231 \end_layout
232
233 \begin_layout Abstract
234 This is a preliminary report on surface photometry of the major fraction
235  of known globular clusters, to see which of them show the signs of a collapsed
236  core.
237  We also explore some diversionary mathematics and recreational tables.
238  
239 \end_layout
240
241 \begin_layout Keywords
242 clusters: globular, peanut---bosons: bozos
243 \end_layout
244
245 \begin_layout Section
246 Introduction
247 \end_layout
248
249 \begin_layout Standard
250 A focal problem today in the dynamics of globular clusters is core collapse.
251  It has been predicted by theory for decades 
252 \begin_inset ERT
253 status collapsed
254
255 \begin_layout Plain Layout
256
257
258 \backslash
259 citep{hen61,lyn68,spi85}
260 \end_layout
261
262 \end_inset
263
264 , but observation has been less alert to the phenomenon.
265  For many years the central brightness peak in M15 
266 \begin_inset ERT
267 status collapsed
268
269 \begin_layout Plain Layout
270
271
272 \backslash
273 citep{kin75,new78}
274 \end_layout
275
276 \end_inset
277
278  seemed a unique anomaly.
279  Then 
280 \begin_inset ERT
281 status collapsed
282
283 \begin_layout Plain Layout
284
285
286 \backslash
287 citet{aur82}
288 \end_layout
289
290 \end_inset
291
292  suggested a central peak in NGC 6397, and a limited photographic survey
293  of ours 
294 \begin_inset ERT
295 status collapsed
296
297 \begin_layout Plain Layout
298
299
300 \backslash
301 citep[Paper I]{djo84}
302 \end_layout
303
304 \end_inset
305
306  found three more cases, including NGC 6624, whose sharp center had often
307  been remarked on 
308 \begin_inset ERT
309 status collapsed
310
311 \begin_layout Plain Layout
312
313
314 \backslash
315 citep{can78}
316 \end_layout
317
318 \end_inset
319
320 .
321  
322 \end_layout
323
324 \begin_layout Section
325 Observations
326 \end_layout
327
328 \begin_layout Standard
329 All our observations were short direct exposures with CCD's.
330  At Lick Observatory we used a TI 500
331 \begin_inset Formula $\times$
332 \end_inset
333
334 500 chip and a GEC 575
335 \begin_inset Formula $\times$
336 \end_inset
337
338 385, on the 1-m Nickel reflector.
339  The only filter available at Lick was red.
340  At CTIO we used a GEC 575
341 \begin_inset Formula $\times$
342 \end_inset
343
344 385, with 
345 \begin_inset Formula $B,V,$
346 \end_inset
347
348  and 
349 \begin_inset Formula $R$
350 \end_inset
351
352  filters, and an RCA 512
353 \begin_inset Formula $\times$
354 \end_inset
355
356 320, with 
357 \begin_inset Formula $U,B,V,R,$
358 \end_inset
359
360  and 
361 \begin_inset Formula $I$
362 \end_inset
363
364  filters, on the 1.5-m reflector.
365  In the CTIO observations we tried to concentrate on the shortest practicable
366  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
367  often kept us from observing in 
368 \begin_inset Formula $U$
369 \end_inset
370
371  or even in 
372 \begin_inset Formula $B$
373 \end_inset
374
375 .
376  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
377  sizes were around 3 arcmin.
378 \end_layout
379
380 \begin_layout Standard
381 The CCD images are unfortunately not always suitable, for very poor clusters
382  or for clusters with large cores.
383  Since the latter are easily studied by other means, we augmented our own
384  CCD profiles by collecting from the literature a number of star-count profiles
385  
386 \begin_inset ERT
387 status collapsed
388
389 \begin_layout Plain Layout
390
391
392 \backslash
393 citep{kin68,pet76,har84,ort85}
394 \end_layout
395
396 \end_inset
397
398 , as well as photoelectric profiles 
399 \begin_inset ERT
400 status collapsed
401
402 \begin_layout Plain Layout
403
404
405 \backslash
406 citep{kin66,kin75}
407 \end_layout
408
409 \end_inset
410
411  and electronographic profiles 
412 \begin_inset ERT
413 status collapsed
414
415 \begin_layout Plain Layout
416
417
418 \backslash
419 citep{kro84}
420 \end_layout
421
422 \end_inset
423
424 .
425  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
426 \end_layout
427
428 \begin_layout Section
429 Helicity Amplitudes
430 \end_layout
431
432 \begin_layout Standard
433 It has been realized that helicity amplitudes provide a convenient means
434  for Feynman diagram
435 \begin_inset Foot
436 status collapsed
437
438 \begin_layout Plain Layout
439 Footnotes can be inserted like this.
440 \end_layout
441
442 \end_inset
443
444  evaluations.
445  These amplitude-level techniques are particularly convenient for calculations
446  involving many Feynman diagrams, where the usual trace techniques for the
447  amplitude squared becomes unwieldy.
448  Our calculations use the helicity techniques developed by other authors
449  
450 \begin_inset CommandInset citation
451 LatexCommand cite
452 key "hag86"
453
454 \end_inset
455
456 ; we briefly summarize below.
457 \end_layout
458
459 \begin_layout Subsection
460 Formalism
461 \end_layout
462
463 \begin_layout Standard
464 \begin_inset CommandInset label
465 LatexCommand label
466 name "bozomath"
467
468 \end_inset
469
470
471 \end_layout
472
473 \begin_layout Standard
474 A tree-level amplitude in 
475 \begin_inset Formula $e^{+}e^{-}$
476 \end_inset
477
478  collisions can be expressed in terms of fermion strings of the form 
479 \begin_inset Formula 
480 \begin{equation}
481 \bar{v}(p_{2},\sigma_{2})P_{-\tau}\hat{a}_{1}\hat{a}_{2}\cdots\hat{a}_{n}u(p_{1},\sigma_{1}),
482 \end{equation}
483
484 \end_inset
485
486  where 
487 \begin_inset Formula $p$
488 \end_inset
489
490  and 
491 \begin_inset Formula $\sigma$
492 \end_inset
493
494  label the initial 
495 \begin_inset Formula $e^{\pm}$
496 \end_inset
497
498  four-momenta and helicities 
499 \begin_inset Formula $(\sigma=\pm1)$
500 \end_inset
501
502
503 \begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
504 \end_inset
505
506  and 
507 \begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
508 \end_inset
509
510  is a chirality projection operator 
511 \begin_inset Formula $(\tau=\pm1)$
512 \end_inset
513
514 .
515  The 
516 \begin_inset Formula $a_{i}^{\mu}$
517 \end_inset
518
519  may be formed from particle four-momenta, gauge-boson polarization vectors
520  or fermion strings with an uncontracted Lorentz index associated with final-sta
521 te fermions.
522 \end_layout
523
524 \begin_layout NoteToEditor
525 Figures 1 and 2 should appear side-by-side in print
526 \end_layout
527
528 \begin_layout Standard
529 In the chiral representation the 
530 \begin_inset Formula $\gamma$
531 \end_inset
532
533  matrices are expressed in terms of 
534 \begin_inset Formula $2\times2$
535 \end_inset
536
537  Pauli matrices 
538 \begin_inset Formula $\sigma$
539 \end_inset
540
541  and the unit matrix 1 as 
542 \begin_inset Formula 
543 \begin{eqnarray*}
544 \gamma^{\mu} & = & \left(\begin{array}{cc}
545 0 & \sigma_{+}^{\mu}\\
546 \sigma_{-}^{\mu} & 0
547 \end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
548 -1 & 0\\
549 0 & 1
550 \end{array}\right),\\
551 \sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),
552 \end{eqnarray*}
553
554 \end_inset
555
556  giving 
557 \begin_inset Formula 
558 \begin{equation}
559 \hat{a}=\left(\begin{array}{cc}
560 0 & (\hat{a})_{+}\\
561 (\hat{a})_{-} & 0
562 \end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},
563 \end{equation}
564
565 \end_inset
566
567  The spinors are expressed in terms of two-component Weyl spinors as 
568 \begin_inset Formula 
569 \begin{equation}
570 u=\left(\begin{array}{c}
571 (u)_{-}\\
572 (u)_{+}
573 \end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.
574 \end{equation}
575
576 \end_inset
577
578
579 \end_layout
580
581 \begin_layout Standard
582 The Weyl spinors are given in terms of helicity eigenstates 
583 \begin_inset Formula $\chi_{\lambda}(p)$
584 \end_inset
585
586  with 
587 \begin_inset Formula $\lambda=\pm1$
588 \end_inset
589
590  by 
591 \end_layout
592
593 \begin_layout MathLetters
594 \begin_inset Formula 
595 \begin{eqnarray}
596 u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
597 v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)
598 \end{eqnarray}
599
600 \end_inset
601
602
603 \end_layout
604
605 \begin_layout Section
606 Floating material and so forth
607 \end_layout
608
609 \begin_layout Standard
610 Consider a task that computes profile parameters for a modified Lorentzian
611  of the form 
612 \begin_inset Formula 
613 \begin{equation}
614 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
615 \end{equation}
616
617 \end_inset
618
619  where 
620 \begin_inset Formula 
621 \[
622 d_{1}=\sqrt{\left(\begin{array}{c}
623 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
624 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
625 \]
626
627 \end_inset
628
629
630 \begin_inset Formula 
631 \[
632 d_{2}=\sqrt{\left(\begin{array}{c}
633 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
634 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
635 \]
636
637 \end_inset
638
639
640 \begin_inset Formula 
641 \[
642 x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta
643 \]
644
645 \end_inset
646
647
648 \begin_inset Formula 
649 \[
650 y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
651 \]
652
653 \end_inset
654
655
656 \end_layout
657
658 \begin_layout Standard
659 In these expressions 
660 \begin_inset Formula $x_{0}$
661 \end_inset
662
663 ,
664 \begin_inset Formula $y_{0}$
665 \end_inset
666
667  is the star center, and 
668 \begin_inset Formula $\Theta$
669 \end_inset
670
671  is the angle with the 
672 \begin_inset Formula $x$
673 \end_inset
674
675  axis.
676  Results of this task are shown in table
677 \begin_inset space ~
678 \end_inset
679
680
681 \begin_inset CommandInset ref
682 LatexCommand ref
683 reference "tbl-2"
684
685 \end_inset
686
687 .
688  It is not clear how these sorts of analyses may affect determination of
689  
690 \begin_inset Formula $M_{\sun}$
691 \end_inset
692
693 , but the assumption is that the alternate results should be less than 90°
694  out of phase with previous values.
695  We have no observations of 
696 \begin_inset ERT
697 status collapsed
698
699 \begin_layout Plain Layout
700
701
702 \backslash
703 ion{Ca}{2}
704 \end_layout
705
706 \end_inset
707
708 .
709  Roughly 
710 \begin_inset ERT
711 status collapsed
712
713 \begin_layout Plain Layout
714
715
716 \backslash
717 slantfrac{4}{5}
718 \end_layout
719
720 \end_inset
721
722  of the electronically submitted abstracts for AAS meetings are error-free.
723 \end_layout
724
725 \begin_layout Acknowledgements
726
727 \end_layout
728
729 \begin_layout Standard
730 We are grateful to V.
731  Barger, T.
732  Han, and R.
733  J.
734  N.
735  Phillips for doing the math in section
736 \begin_inset space ~
737 \end_inset
738
739
740 \begin_inset CommandInset ref
741 LatexCommand ref
742 reference "bozomath"
743
744 \end_inset
745
746 .
747  More information on the AASTeX macros package are available at 
748 \begin_inset Flex URL
749 status collapsed
750
751 \begin_layout Plain Layout
752
753 http://www.aas.org/publications/aastex
754 \end_layout
755
756 \end_inset
757
758  or the 
759 \begin_inset ERT
760 status collapsed
761
762 \begin_layout Plain Layout
763
764
765 \backslash
766 anchor{
767 \end_layout
768
769 \end_inset
770
771 ftp://www.aas.org/pubs/
772 \begin_inset ERT
773 status collapsed
774
775 \begin_layout Plain Layout
776
777 }{
778 \end_layout
779
780 \end_inset
781
782 AAS ftp site
783 \begin_inset ERT
784 status collapsed
785
786 \begin_layout Plain Layout
787
788 }
789 \end_layout
790
791 \end_inset
792
793 .
794 \end_layout
795
796 \begin_layout Appendix
797
798 \end_layout
799
800 \begin_layout Section
801 Appendicial material
802 \end_layout
803
804 \begin_layout Standard
805 Consider once again a task that computes profile parameters for a modified
806  Lorentzian of the form 
807 \begin_inset Formula 
808 \begin{equation}
809 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
810 \end{equation}
811
812 \end_inset
813
814  where 
815 \end_layout
816
817 \begin_layout MathLetters
818 \begin_inset Formula 
819 \[
820 d_{1}=\frac{3}{4}\sqrt{\left(\begin{array}{c}
821 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
822 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
823 \]
824
825 \end_inset
826
827
828 \begin_inset Formula 
829 \begin{equation}
830 d_{2}=\case{3}{4}\sqrt{\left(\begin{array}{c}
831 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
832 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
833 \end{equation}
834
835 \end_inset
836
837
838 \begin_inset Formula 
839 \begin{eqnarray}
840 x_{1} & = & (x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\\
841 y_{1} & = & -(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
842 \end{eqnarray}
843
844 \end_inset
845
846
847 \end_layout
848
849 \begin_layout Standard
850 For completeness, here is one last equation.
851  
852 \begin_inset Formula 
853 \begin{equation}
854 e=mc^{2}
855 \end{equation}
856
857 \end_inset
858
859
860 \end_layout
861
862 \begin_layout References
863 \begin_inset CommandInset bibitem
864 LatexCommand bibitem
865 label "Auri\\`ere(1982)"
866 key "aur82"
867
868 \end_inset
869
870 Aurière, M.
871  1982, 
872 \begin_inset ERT
873 status collapsed
874
875 \begin_layout Plain Layout
876
877
878 \backslash
879 aap
880 \end_layout
881
882 \end_inset
883
884 , 109, 301 
885 \end_layout
886
887 \begin_layout References
888 \begin_inset CommandInset bibitem
889 LatexCommand bibitem
890 label "Canizares et al.(1978)"
891 key "can78"
892
893 \end_inset
894
895 Canizares, C.
896  R., Grindlay, J.
897  E., Hiltner, W.
898  A., Liller, W., and McClintock, J.
899  E.
900  1978, 
901 \begin_inset ERT
902 status collapsed
903
904 \begin_layout Plain Layout
905
906
907 \backslash
908 apj
909 \end_layout
910
911 \end_inset
912
913 , 224, 39 
914 \end_layout
915
916 \begin_layout References
917 \begin_inset CommandInset bibitem
918 LatexCommand bibitem
919 label "Djorgovski and King(1984)"
920 key "djo84"
921
922 \end_inset
923
924 Djorgovski, S., and King, I.
925  R.
926  1984, 
927 \begin_inset ERT
928 status collapsed
929
930 \begin_layout Plain Layout
931
932
933 \backslash
934 apjl
935 \end_layout
936
937 \end_inset
938
939 , 277, L49 
940 \end_layout
941
942 \begin_layout References
943 \begin_inset CommandInset bibitem
944 LatexCommand bibitem
945 label "Hagiwara and Zeppenfeld(1986)"
946 key "hag86"
947
948 \end_inset
949
950 Hagiwara, K., and Zeppenfeld, D.
951  1986, Nucl.Phys., 274, 1 
952 \end_layout
953
954 \begin_layout References
955 \begin_inset CommandInset bibitem
956 LatexCommand bibitem
957 label "Harris and van den Bergh(1984)"
958 key "har84"
959
960 \end_inset
961
962 Harris, W.
963  E., and van den Bergh, S.
964  1984, 
965 \begin_inset ERT
966 status collapsed
967
968 \begin_layout Plain Layout
969
970
971 \backslash
972 aj
973 \end_layout
974
975 \end_inset
976
977 , 89, 1816 
978 \end_layout
979
980 \begin_layout References
981 \begin_inset CommandInset bibitem
982 LatexCommand bibitem
983 label "H\\`enon(1961)"
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985
986 \end_inset
987
988 Hénon, M.
989  1961, Ann.d'Ap., 24, 369 
990 \end_layout
991
992 \begin_layout References
993 \begin_inset CommandInset bibitem
994 LatexCommand bibitem
995 label "King(1966)"
996 key "kin66"
997
998 \end_inset
999
1000 King, I.
1001  R.
1002  1966, 
1003 \begin_inset ERT
1004 status collapsed
1005
1006 \begin_layout Plain Layout
1007
1008
1009 \backslash
1010 aj
1011 \end_layout
1012
1013 \end_inset
1014
1015 , 71, 276 
1016 \end_layout
1017
1018 \begin_layout References
1019 \begin_inset CommandInset bibitem
1020 LatexCommand bibitem
1021 label "King(1975)"
1022 key "kin75"
1023
1024 \end_inset
1025
1026 King, I.
1027  R.
1028  1975, Dynamics of Stellar Systems, A.
1029  Hayli, Dordrecht: Reidel, 1975, 99 
1030 \end_layout
1031
1032 \begin_layout References
1033 \begin_inset CommandInset bibitem
1034 LatexCommand bibitem
1035 label "King et al.(1968)"
1036 key "kin68"
1037
1038 \end_inset
1039
1040 King, I.
1041  R., Hedemann, E., Hodge, S.
1042  M., and White, R.
1043  E.
1044  1968, 
1045 \begin_inset ERT
1046 status collapsed
1047
1048 \begin_layout Plain Layout
1049
1050
1051 \backslash
1052 aj
1053 \end_layout
1054
1055 \end_inset
1056
1057 , 73, 456 
1058 \end_layout
1059
1060 \begin_layout References
1061 \begin_inset CommandInset bibitem
1062 LatexCommand bibitem
1063 label "Kron et al.(1984)"
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1065
1066 \end_inset
1067
1068 Kron, G.
1069  E., Hewitt, A.
1070  V., and Wasserman, L.
1071  H.
1072  1984, 
1073 \begin_inset ERT
1074 status collapsed
1075
1076 \begin_layout Plain Layout
1077
1078
1079 \backslash
1080 pasp
1081 \end_layout
1082
1083 \end_inset
1084
1085 , 96, 198 
1086 \end_layout
1087
1088 \begin_layout References
1089 \begin_inset CommandInset bibitem
1090 LatexCommand bibitem
1091 label "Lynden-Bell and Wood(1968)"
1092 key "lyn68"
1093
1094 \end_inset
1095
1096 Lynden-Bell, D., and Wood, R.
1097  1968, 
1098 \begin_inset ERT
1099 status collapsed
1100
1101 \begin_layout Plain Layout
1102
1103
1104 \backslash
1105 mnras
1106 \end_layout
1107
1108 \end_inset
1109
1110 , 138, 495 
1111 \end_layout
1112
1113 \begin_layout References
1114 \begin_inset CommandInset bibitem
1115 LatexCommand bibitem
1116 label "Newell and O'Neil(1978)"
1117 key "new78"
1118
1119 \end_inset
1120
1121 Newell, E.
1122  B., and O'Neil, E.
1123  J.
1124  1978, 
1125 \begin_inset ERT
1126 status collapsed
1127
1128 \begin_layout Plain Layout
1129
1130
1131 \backslash
1132 apjs
1133 \end_layout
1134
1135 \end_inset
1136
1137 , 37, 27 
1138 \end_layout
1139
1140 \begin_layout References
1141 \begin_inset CommandInset bibitem
1142 LatexCommand bibitem
1143 label "Ortolani et al.(1985)"
1144 key "ort85"
1145
1146 \end_inset
1147
1148 Ortolani, S., Rosino, L., and Sandage, A.
1149  1985, 
1150 \begin_inset ERT
1151 status collapsed
1152
1153 \begin_layout Plain Layout
1154
1155
1156 \backslash
1157 aj
1158 \end_layout
1159
1160 \end_inset
1161
1162 , 90, 473 
1163 \end_layout
1164
1165 \begin_layout References
1166 \begin_inset CommandInset bibitem
1167 LatexCommand bibitem
1168 label "Peterson(1976)"
1169 key "pet76"
1170
1171 \end_inset
1172
1173 Peterson, C.
1174  J.
1175  1976, 
1176 \begin_inset ERT
1177 status collapsed
1178
1179 \begin_layout Plain Layout
1180
1181
1182 \backslash
1183 aj
1184 \end_layout
1185
1186 \end_inset
1187
1188 , 81, 617 
1189 \end_layout
1190
1191 \begin_layout References
1192 \begin_inset CommandInset bibitem
1193 LatexCommand bibitem
1194 label "Spitzer(1985)"
1195 key "spi85"
1196
1197 \end_inset
1198
1199 Spitzer, L.
1200  1985, Dynamics of Star Clusters, J.
1201  Goodman and P.
1202  Hut, Dordrecht: Reidel, 109 
1203 \end_layout
1204
1205 \begin_layout Standard
1206 \begin_inset Newpage clearpage
1207 \end_inset
1208
1209
1210 \end_layout
1211
1212 \begin_layout Standard
1213 \begin_inset Caption FigCaption
1214
1215 \begin_layout Plain Layout
1216 \begin_inset CommandInset label
1217 LatexCommand label
1218 name "fig1"
1219
1220 \end_inset
1221
1222 This is the first figure and it uses sgi9259.eps as its EPS figure file.
1223 \end_layout
1224
1225 \end_inset
1226
1227
1228 \end_layout
1229
1230 \begin_layout Standard
1231 \begin_inset Caption FigCaption
1232
1233 \begin_layout Plain Layout
1234 \begin_inset CommandInset label
1235 LatexCommand label
1236 name "fig2"
1237
1238 \end_inset
1239
1240 This is an example of a long figure caption that must be set as a paragraph.
1241   The processor has to buffer the text of the caption, so it is good not
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1243  
1244 \end_layout
1245
1246 \end_inset
1247
1248
1249 \end_layout
1250
1251 \begin_layout Standard
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1253
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1255 \begin_inset CommandInset label
1256 LatexCommand label
1257 name "fig3"
1258
1259 \end_inset
1260
1261 This figure has no associated EPS file, so the optional parameter is omitted.
1262  
1263 \end_layout
1264
1265 \end_inset
1266
1267
1268 \end_layout
1269
1270 \begin_layout Standard
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1272 \end_inset
1273
1274
1275 \end_layout
1276
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1281 status open
1282
1283 \begin_layout Plain Layout
1284 \begin_inset Caption Standard
1285
1286 \begin_layout Plain Layout
1287 Terribly relevant tabular information.
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1289 LatexCommand label
1290 name "tbl-2"
1291
1292 \end_inset
1293
1294
1295 \end_layout
1296
1297 \end_inset
1298
1299
1300 \end_layout
1301
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1305
1306
1307 \end_layout
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1330
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1339
1340 \begin_layout Plain Layout
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1353
1354
1355 \end_layout
1356
1357 \end_inset
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1361
1362 \begin_layout Plain Layout
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1366
1367
1368 \end_layout
1369
1370 \end_inset
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1379
1380
1381 \end_layout
1382
1383 \end_inset
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1393
1394 \end_layout
1395
1396 \end_inset
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1405
1406
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1408
1409 \end_inset
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1418
1419
1420 \end_layout
1421
1422 \end_inset
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1432 \begin_inset Flex tablenotemark
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1434
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1438
1439 \end_inset
1440
1441
1442 \end_layout
1443
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1453
1454
1455 \end_layout
1456
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1462 \begin_layout Plain Layout
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1466
1467
1468 \end_layout
1469
1470 \end_inset
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1486
1487 \end_inset
1488
1489
1490 \end_layout
1491
1492 \end_inset
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1514
1515 \backslash
1516 tableline
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1518 tableline
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1520
1521 \end_inset
1522
1523
1524 \end_layout
1525
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1531 \begin_layout Plain Layout
1532 33472.5 
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1534
1535 \end_inset
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1540 \begin_layout Plain Layout
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1549 \begin_layout Plain Layout
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1552
1553 \end_inset
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1557
1558 \begin_layout Plain Layout
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1562 \end_inset
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1567 \begin_layout Plain Layout
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1591 <cell alignment="right" valignment="top" usebox="none">
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1604 68.3 
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1631 1,2
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1773 \end_inset
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1775 <cell alignment="right" valignment="top" usebox="none">
1776 \begin_inset Text
1777
1778 \begin_layout Plain Layout
1779 0.9 
1780 \end_layout
1781
1782 \end_inset
1783 </cell>
1784 <cell alignment="right" valignment="top" usebox="none">
1785 \begin_inset Text
1786
1787 \begin_layout Plain Layout
1788 0.3 
1789 \end_layout
1790
1791 \end_inset
1792 </cell>
1793 <cell alignment="right" valignment="top" usebox="none">
1794 \begin_inset Text
1795
1796 \begin_layout Plain Layout
1797 60 
1798 \end_layout
1799
1800 \end_inset
1801 </cell>
1802 <cell alignment="right" valignment="top" usebox="none">
1803 \begin_inset Text
1804
1805 \begin_layout Plain Layout
1806 3.4 
1807 \end_layout
1808
1809 \end_inset
1810 </cell>
1811 <cell alignment="right" valignment="top" usebox="none">
1812 \begin_inset Text
1813
1814 \begin_layout Plain Layout
1815 1.622 
1816 \end_layout
1817
1818 \end_inset
1819 </cell>
1820 <cell alignment="right" valignment="top" usebox="none">
1821 \begin_inset Text
1822
1823 \begin_layout Plain Layout
1824 1.551 
1825 \end_layout
1826
1827 \end_inset
1828 </cell>
1829 <cell alignment="right" valignment="top" usebox="none">
1830 \begin_inset Text
1831
1832 \begin_layout Plain Layout
1833 2.159 
1834 \end_layout
1835
1836 \end_inset
1837 </cell>
1838 <cell alignment="right" valignment="top" usebox="none">
1839 \begin_inset Text
1840
1841 \begin_layout Plain Layout
1842 6.7 
1843 \end_layout
1844
1845 \end_inset
1846 </cell>
1847 <cell alignment="right" valignment="top" usebox="none">
1848 \begin_inset Text
1849
1850 \begin_layout Plain Layout
1851 7.3 
1852 \end_layout
1853
1854 \end_inset
1855 </cell>
1856 <cell alignment="right" valignment="top" usebox="none">
1857 \begin_inset Text
1858
1859 \begin_layout Plain Layout
1860 -40.272
1861 \end_layout
1862
1863 \end_inset
1864 </cell>
1865 <cell alignment="right" valignment="top" usebox="none">
1866 \begin_inset Text
1867
1868 \begin_layout Plain Layout
1869 4
1870 \end_layout
1871
1872 \end_inset
1873 </cell>
1874 </row>
1875 <row>
1876 <cell alignment="center" valignment="top" usebox="none">
1877 \begin_inset Text
1878
1879 \begin_layout Plain Layout
1880  4 
1881 \end_layout
1882
1883 \end_inset
1884 </cell>
1885 <cell alignment="right" valignment="top" usebox="none">
1886 \begin_inset Text
1887
1888 \begin_layout Plain Layout
1889 32733.8 
1890 \end_layout
1891
1892 \end_inset
1893 </cell>
1894 <cell alignment="right" valignment="top" usebox="none">
1895 \begin_inset Text
1896
1897 \begin_layout Plain Layout
1898 -1.2
1899 \begin_inset Flex tablenotemark
1900 status open
1901
1902 \begin_layout Plain Layout
1903 c
1904 \end_layout
1905
1906 \end_inset
1907
1908
1909 \end_layout
1910
1911 \end_inset
1912 </cell>
1913 <cell alignment="right" valignment="top" usebox="none">
1914 \begin_inset Text
1915
1916 \begin_layout Plain Layout
1917 -0.5 
1918 \end_layout
1919
1920 \end_inset
1921 </cell>
1922 <cell alignment="right" valignment="top" usebox="none">
1923 \begin_inset Text
1924
1925 \begin_layout Plain Layout
1926 41 
1927 \end_layout
1928
1929 \end_inset
1930 </cell>
1931 <cell alignment="right" valignment="top" usebox="none">
1932 \begin_inset Text
1933
1934 \begin_layout Plain Layout
1935 54.8 
1936 \end_layout
1937
1938 \end_inset
1939 </cell>
1940 <cell alignment="right" valignment="top" usebox="none">
1941 \begin_inset Text
1942
1943 \begin_layout Plain Layout
1944 2.282 
1945 \end_layout
1946
1947 \end_inset
1948 </cell>
1949 <cell alignment="right" valignment="top" usebox="none">
1950 \begin_inset Text
1951
1952 \begin_layout Plain Layout
1953 2.156 
1954 \end_layout
1955
1956 \end_inset
1957 </cell>
1958 <cell alignment="right" valignment="top" usebox="none">
1959 \begin_inset Text
1960
1961 \begin_layout Plain Layout
1962 4.313 
1963 \end_layout
1964
1965 \end_inset
1966 </cell>
1967 <cell alignment="right" valignment="top" usebox="none">
1968 \begin_inset Text
1969
1970 \begin_layout Plain Layout
1971 117.4 
1972 \end_layout
1973
1974 \end_inset
1975 </cell>
1976 <cell alignment="right" valignment="top" usebox="none">
1977 \begin_inset Text
1978
1979 \begin_layout Plain Layout
1980 78.2 
1981 \end_layout
1982
1983 \end_inset
1984 </cell>
1985 <cell alignment="right" valignment="top" usebox="none">
1986 \begin_inset Text
1987
1988 \begin_layout Plain Layout
1989 -35.847
1990 \end_layout
1991
1992 \end_inset
1993 </cell>
1994 <cell alignment="right" valignment="top" usebox="none">
1995 \begin_inset Text
1996
1997 \begin_layout Plain Layout
1998 5,6
1999 \end_layout
2000
2001 \end_inset
2002 </cell>
2003 </row>
2004 <row>
2005 <cell alignment="center" valignment="top" usebox="none">
2006 \begin_inset Text
2007
2008 \begin_layout Plain Layout
2009  5 
2010 \end_layout
2011
2012 \end_inset
2013 </cell>
2014 <cell alignment="right" valignment="top" usebox="none">
2015 \begin_inset Text
2016
2017 \begin_layout Plain Layout
2018  9607.4 
2019 \end_layout
2020
2021 \end_inset
2022 </cell>
2023 <cell alignment="right" valignment="top" usebox="none">
2024 \begin_inset Text
2025
2026 \begin_layout Plain Layout
2027 -0.4 
2028 \end_layout
2029
2030 \end_inset
2031 </cell>
2032 <cell alignment="right" valignment="top" usebox="none">
2033 \begin_inset Text
2034
2035 \begin_layout Plain Layout
2036 -0.4 
2037 \end_layout
2038
2039 \end_inset
2040 </cell>
2041 <cell alignment="right" valignment="top" usebox="none">
2042 \begin_inset Text
2043
2044 \begin_layout Plain Layout
2045 60 
2046 \end_layout
2047
2048 \end_inset
2049 </cell>
2050 <cell alignment="right" valignment="top" usebox="none">
2051 \begin_inset Text
2052
2053 \begin_layout Plain Layout
2054 1.4 
2055 \end_layout
2056
2057 \end_inset
2058 </cell>
2059 <cell alignment="right" valignment="top" usebox="none">
2060 \begin_inset Text
2061
2062 \begin_layout Plain Layout
2063 1.669
2064 \begin_inset Flex tablenotemark
2065 status collapsed
2066
2067 \begin_layout Plain Layout
2068 c
2069 \end_layout
2070
2071 \end_inset
2072
2073
2074 \end_layout
2075
2076 \end_inset
2077 </cell>
2078 <cell alignment="right" valignment="top" usebox="none">
2079 \begin_inset Text
2080
2081 \begin_layout Plain Layout
2082 1.574 
2083 \end_layout
2084
2085 \end_inset
2086 </cell>
2087 <cell alignment="right" valignment="top" usebox="none">
2088 \begin_inset Text
2089
2090 \begin_layout Plain Layout
2091 2.343 
2092 \end_layout
2093
2094 \end_inset
2095 </cell>
2096 <cell alignment="right" valignment="top" usebox="none">
2097 \begin_inset Text
2098
2099 \begin_layout Plain Layout
2100 8.0 
2101 \end_layout
2102
2103 \end_inset
2104 </cell>
2105 <cell alignment="right" valignment="top" usebox="none">
2106 \begin_inset Text
2107
2108 \begin_layout Plain Layout
2109 8.9 
2110 \end_layout
2111
2112 \end_inset
2113 </cell>
2114 <cell alignment="right" valignment="top" usebox="none">
2115 \begin_inset Text
2116
2117 \begin_layout Plain Layout
2118 -33.417
2119 \end_layout
2120
2121 \end_inset
2122 </cell>
2123 <cell alignment="right" valignment="top" usebox="none">
2124 \begin_inset Text
2125
2126 \begin_layout Plain Layout
2127 7
2128 \end_layout
2129
2130 \end_inset
2131 </cell>
2132 </row>
2133 <row>
2134 <cell alignment="center" valignment="top" usebox="none">
2135 \begin_inset Text
2136
2137 \begin_layout Plain Layout
2138  6 
2139 \end_layout
2140
2141 \end_inset
2142 </cell>
2143 <cell alignment="right" valignment="top" usebox="none">
2144 \begin_inset Text
2145
2146 \begin_layout Plain Layout
2147 31638.6 
2148 \end_layout
2149
2150 \end_inset
2151 </cell>
2152 <cell alignment="right" valignment="top" usebox="none">
2153 \begin_inset Text
2154
2155 \begin_layout Plain Layout
2156 1.6 
2157 \end_layout
2158
2159 \end_inset
2160 </cell>
2161 <cell alignment="right" valignment="top" usebox="none">
2162 \begin_inset Text
2163
2164 \begin_layout Plain Layout
2165 0.1 
2166 \end_layout
2167
2168 \end_inset
2169 </cell>
2170 <cell alignment="right" valignment="top" usebox="none">
2171 \begin_inset Text
2172
2173 \begin_layout Plain Layout
2174 39 
2175 \end_layout
2176
2177 \end_inset
2178 </cell>
2179 <cell alignment="right" valignment="top" usebox="none">
2180 \begin_inset Text
2181
2182 \begin_layout Plain Layout
2183 315.2 
2184 \end_layout
2185
2186 \end_inset
2187 </cell>
2188 <cell alignment="right" valignment="top" usebox="none">
2189 \begin_inset Text
2190
2191 \begin_layout Plain Layout
2192  3.433 
2193 \end_layout
2194
2195 \end_inset
2196 </cell>
2197 <cell alignment="right" valignment="top" usebox="none">
2198 \begin_inset Text
2199
2200 \begin_layout Plain Layout
2201 3.075 
2202 \end_layout
2203
2204 \end_inset
2205 </cell>
2206 <cell alignment="right" valignment="top" usebox="none">
2207 \begin_inset Text
2208
2209 \begin_layout Plain Layout
2210 7.488 
2211 \end_layout
2212
2213 \end_inset
2214 </cell>
2215 <cell alignment="right" valignment="top" usebox="none">
2216 \begin_inset Text
2217
2218 \begin_layout Plain Layout
2219 92.1 
2220 \end_layout
2221
2222 \end_inset
2223 </cell>
2224 <cell alignment="right" valignment="top" usebox="none">
2225 \begin_inset Text
2226
2227 \begin_layout Plain Layout
2228 25.3 
2229 \end_layout
2230
2231 \end_inset
2232 </cell>
2233 <cell alignment="right" valignment="top" usebox="none">
2234 \begin_inset Text
2235
2236 \begin_layout Plain Layout
2237 -12.052 
2238 \end_layout
2239
2240 \end_inset
2241 </cell>
2242 <cell alignment="right" valignment="top" usebox="none">
2243 \begin_inset Text
2244
2245 \begin_layout Plain Layout
2246 8
2247 \end_layout
2248
2249 \end_inset
2250 </cell>
2251 </row>
2252 </lyxtabular>
2253
2254 \end_inset
2255
2256
2257 \end_layout
2258
2259 \begin_layout Table note
2260 a
2261 \begin_inset ERT
2262 status collapsed
2263
2264 \begin_layout Plain Layout
2265
2266 }{
2267 \end_layout
2268
2269 \end_inset
2270
2271 Sample footnote for table
2272 \begin_inset space ~
2273 \end_inset
2274
2275
2276 \begin_inset CommandInset ref
2277 LatexCommand ref
2278 reference "tbl-2"
2279
2280 \end_inset
2281
2282  that was generated with the LaTeX table environment
2283 \end_layout
2284
2285 \begin_layout Table note
2286 b
2287 \begin_inset ERT
2288 status collapsed
2289
2290 \begin_layout Plain Layout
2291
2292 }{
2293 \end_layout
2294
2295 \end_inset
2296
2297 Yet another sample footnote for table
2298 \begin_inset space ~
2299 \end_inset
2300
2301
2302 \begin_inset CommandInset ref
2303 LatexCommand ref
2304 reference "tbl-2"
2305
2306 \end_inset
2307
2308
2309 \end_layout
2310
2311 \begin_layout Table note
2312 c
2313 \begin_inset ERT
2314 status collapsed
2315
2316 \begin_layout Plain Layout
2317
2318 }{
2319 \end_layout
2320
2321 \end_inset
2322
2323 Another sample footnote for table
2324 \begin_inset space ~
2325 \end_inset
2326
2327
2328 \begin_inset CommandInset ref
2329 LatexCommand ref
2330 reference "tbl-2"
2331
2332 \end_inset
2333
2334
2335 \end_layout
2336
2337 \begin_layout TableComments
2338 We can also attach a long-ish paragraph of explanatory material to a table.
2339  Use 
2340 \backslash
2341 tablerefs to append a list of references.
2342  The following references were from a different table: I've patched them
2343  in here to show how they look, but don't take them too seriously---I certainly
2344  have not.
2345 \end_layout
2346
2347 \begin_layout TableRefs
2348 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
2349  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
2350  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
2351  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
2352  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
2353  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
2354  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
2355  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
2356  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
2357  al.
2358  1991; (26) Olsen 1983.
2359 \end_layout
2360
2361 \end_inset
2362
2363
2364 \end_layout
2365
2366 \begin_layout Standard
2367 \begin_inset ERT
2368 status collapsed
2369
2370 \begin_layout Plain Layout
2371
2372 % LyX can load deluxetable files verbatim.
2373  To see this in action, uncomment the following
2374 \end_layout
2375
2376 \end_inset
2377
2378
2379 \end_layout
2380
2381 \begin_layout Standard
2382 \begin_inset ERT
2383 status collapsed
2384
2385 \begin_layout Plain Layout
2386
2387 % line (delete the 
2388 \end_layout
2389
2390 \end_inset
2391
2392
2393 \begin_inset Quotes eld
2394 \end_inset
2395
2396
2397 \begin_inset ERT
2398 status collapsed
2399
2400 \begin_layout Plain Layout
2401
2402 %
2403 \end_layout
2404
2405 \end_inset
2406
2407
2408 \begin_inset Quotes erd
2409 \end_inset
2410
2411
2412 \begin_inset ERT
2413 status collapsed
2414
2415 \begin_layout Plain Layout
2416
2417 ) and copy the file table.tex from the AASTeX 5.0 distribution into
2418 \end_layout
2419
2420 \end_inset
2421
2422
2423 \end_layout
2424
2425 \begin_layout Standard
2426 \begin_inset ERT
2427 status collapsed
2428
2429 \begin_layout Plain Layout
2430
2431 % the same directory as this file.
2432 \end_layout
2433
2434 \end_inset
2435
2436
2437 \end_layout
2438
2439 \begin_layout Standard
2440 \begin_inset ERT
2441 status collapsed
2442
2443 \begin_layout Plain Layout
2444
2445 %
2446 \end_layout
2447
2448 \end_inset
2449
2450
2451 \begin_inset CommandInset include
2452 LatexCommand input
2453 filename "table"
2454
2455 \end_inset
2456
2457
2458 \end_layout
2459
2460 \end_body
2461 \end_document