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1 #LyX 1.6.0svn created this file. For more info see http://www.lyx.org/
2 \lyxformat 344
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 \language english
15 \inputencoding default
16 \font_roman default
17 \font_sans default
18 \font_typewriter default
19 \font_default_family default
20 \font_sc false
21 \font_osf false
22 \font_sf_scale 100
23 \font_tt_scale 100
24
25 \graphics default
26 \paperfontsize default
27 \spacing single
28 \use_hyperref false
29 \papersize default
30 \use_geometry false
31 \use_amsmath 0
32 \use_esint 0
33 \cite_engine basic
34 \use_bibtopic false
35 \paperorientation portrait
36 \secnumdepth 3
37 \tocdepth 3
38 \paragraph_separation indent
39 \defskip medskip
40 \quotes_language english
41 \papercolumns 1
42 \papersides 1
43 \paperpagestyle default
44 \tracking_changes false
45 \output_changes false
46 \author "" 
47 \author "" 
48 \end_header
49
50 \begin_body
51
52 \begin_layout Title
53 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
54  Examples
55 \end_layout
56
57 \begin_layout Author
58 S.
59  Djorgovski
60 \begin_inset ERT
61 status collapsed
62
63 \begin_layout Plain Layout
64
65
66 \backslash
67 altaffilmark{1,2,3}
68 \end_layout
69
70 \end_inset
71
72  and Ivan R.
73  King
74 \begin_inset ERT
75 status collapsed
76
77 \begin_layout Plain Layout
78
79
80 \backslash
81 altaffilmark{1}
82 \end_layout
83
84 \end_inset
85
86
87 \end_layout
88
89 \begin_layout Affiliation
90 Astronomy Department, University of California, Berkeley, CA 94720
91 \end_layout
92
93 \begin_layout Author
94 C.
95  D.
96  Biemesderfer
97 \begin_inset ERT
98 status collapsed
99
100 \begin_layout Plain Layout
101
102
103 \backslash
104 altaffilmark{4,5}
105 \end_layout
106
107 \end_inset
108
109
110 \end_layout
111
112 \begin_layout Affiliation
113 National Optical Astronomy Observatories, Tucson, AZ 85719
114 \end_layout
115
116 \begin_layout Email
117 aastex-help@aas.org
118 \end_layout
119
120 \begin_layout And
121
122 \end_layout
123
124 \begin_layout Author
125 R.
126  J.
127  Hanisch
128 \begin_inset ERT
129 status collapsed
130
131 \begin_layout Plain Layout
132
133
134 \backslash
135 altaffilmark{5}
136 \end_layout
137
138 \end_inset
139
140
141 \end_layout
142
143 \begin_layout Affiliation
144 Space Telescope Science Institute, Baltimore, MD 21218
145 \end_layout
146
147 \begin_layout Standard
148 \begin_inset ERT
149 status open
150
151 \begin_layout Plain Layout
152
153
154 \backslash
155 altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
156  CTIO is operated by AURA, Inc.
157 \backslash
158  under contract to the National Science Foundation.} 
159 \end_layout
160
161 \begin_layout Plain Layout
162
163 \end_layout
164
165 \begin_layout Plain Layout
166
167
168 \backslash
169 altaffiltext{2}{Society of Fellows, Harvard University.} 
170 \end_layout
171
172 \begin_layout Plain Layout
173
174 \end_layout
175
176 \begin_layout Plain Layout
177
178
179 \backslash
180 altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
181  Cambridge, MA 02138} 
182 \end_layout
183
184 \begin_layout Plain Layout
185
186 \end_layout
187
188 \begin_layout Plain Layout
189
190
191 \backslash
192 altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
193  
194 \end_layout
195
196 \begin_layout Plain Layout
197
198 \end_layout
199
200 \begin_layout Plain Layout
201
202
203 \backslash
204 altaffiltext{5}{Patron, Alonso's Bar and Grill}
205 \end_layout
206
207 \end_inset
208
209
210 \end_layout
211
212 \begin_layout Abstract
213 This is a preliminary report on surface photometry of the major fraction
214  of known globular clusters, to see which of them show the signs of a collapsed
215  core.
216  We also explore some diversionary mathematics and recreational tables.
217  
218 \end_layout
219
220 \begin_layout Keywords
221 clusters: globular, peanut---bosons: bozos
222 \end_layout
223
224 \begin_layout Section
225 Introduction
226 \end_layout
227
228 \begin_layout Standard
229 A focal problem today in the dynamics of globular clusters is core collapse.
230  It has been predicted by theory for decades 
231 \begin_inset ERT
232 status collapsed
233
234 \begin_layout Plain Layout
235
236
237 \backslash
238 citep{hen61,lyn68,spi85}
239 \end_layout
240
241 \end_inset
242
243 , but observation has been less alert to the phenomenon.
244  For many years the central brightness peak in M15 
245 \begin_inset ERT
246 status collapsed
247
248 \begin_layout Plain Layout
249
250
251 \backslash
252 citep{kin75,new78}
253 \end_layout
254
255 \end_inset
256
257  seemed a unique anomaly.
258  Then 
259 \begin_inset ERT
260 status collapsed
261
262 \begin_layout Plain Layout
263
264
265 \backslash
266 citet{aur82}
267 \end_layout
268
269 \end_inset
270
271  suggested a central peak in NGC 6397, and a limited photographic survey
272  of ours 
273 \begin_inset ERT
274 status collapsed
275
276 \begin_layout Plain Layout
277
278
279 \backslash
280 citep[Paper I]{djo84}
281 \end_layout
282
283 \end_inset
284
285  found three more cases, including NGC 6624, whose sharp center had often
286  been remarked on 
287 \begin_inset ERT
288 status collapsed
289
290 \begin_layout Plain Layout
291
292
293 \backslash
294 citep{can78}
295 \end_layout
296
297 \end_inset
298
299 .
300  
301 \end_layout
302
303 \begin_layout Section
304 Observations
305 \end_layout
306
307 \begin_layout Standard
308 All our observations were short direct exposures with CCD's.
309  At Lick Observatory we used a TI 500
310 \begin_inset Formula $\times$
311 \end_inset
312
313 500 chip and a GEC 575
314 \begin_inset Formula $\times$
315 \end_inset
316
317 385, on the 1-m Nickel reflector.
318  The only filter available at Lick was red.
319  At CTIO we used a GEC 575
320 \begin_inset Formula $\times$
321 \end_inset
322
323 385, with 
324 \begin_inset Formula $B,V,$
325 \end_inset
326
327  and 
328 \begin_inset Formula $R$
329 \end_inset
330
331  filters, and an RCA 512
332 \begin_inset Formula $\times$
333 \end_inset
334
335 320, with 
336 \begin_inset Formula $U,B,V,R,$
337 \end_inset
338
339  and 
340 \begin_inset Formula $I$
341 \end_inset
342
343  filters, on the 1.5-m reflector.
344  In the CTIO observations we tried to concentrate on the shortest practicable
345  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
346  often kept us from observing in 
347 \begin_inset Formula $U$
348 \end_inset
349
350  or even in 
351 \begin_inset Formula $B$
352 \end_inset
353
354 .
355  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
356  sizes were around 3 arcmin.
357 \end_layout
358
359 \begin_layout Standard
360 The CCD images are unfortunately not always suitable, for very poor clusters
361  or for clusters with large cores.
362  Since the latter are easily studied by other means, we augmented our own
363  CCD profiles by collecting from the literature a number of star-count profiles
364  
365 \begin_inset ERT
366 status collapsed
367
368 \begin_layout Plain Layout
369
370
371 \backslash
372 citep{kin68,pet76,har84,ort85}
373 \end_layout
374
375 \end_inset
376
377 , as well as photoelectric profiles 
378 \begin_inset ERT
379 status collapsed
380
381 \begin_layout Plain Layout
382
383
384 \backslash
385 citep{kin66,kin75}
386 \end_layout
387
388 \end_inset
389
390  and electronographic profiles 
391 \begin_inset ERT
392 status collapsed
393
394 \begin_layout Plain Layout
395
396
397 \backslash
398 citep{kro84}
399 \end_layout
400
401 \end_inset
402
403 .
404  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
405 \end_layout
406
407 \begin_layout Section
408 Helicity Amplitudes
409 \end_layout
410
411 \begin_layout Standard
412 It has been realized that helicity amplitudes provide a convenient means
413  for Feynman diagram
414 \begin_inset Foot
415 status collapsed
416
417 \begin_layout Plain Layout
418 Footnotes can be inserted like this.
419 \end_layout
420
421 \end_inset
422
423  evaluations.
424  These amplitude-level techniques are particularly convenient for calculations
425  involving many Feynman diagrams, where the usual trace techniques for the
426  amplitude squared becomes unwieldy.
427  Our calculations use the helicity techniques developed by other authors
428  
429 \begin_inset CommandInset citation
430 LatexCommand cite
431 key "hag86"
432
433 \end_inset
434
435 ; we briefly summarize below.
436 \end_layout
437
438 \begin_layout Subsection
439 Formalism
440 \end_layout
441
442 \begin_layout Standard
443 \begin_inset CommandInset label
444 LatexCommand label
445 name "bozomath"
446
447 \end_inset
448
449
450 \end_layout
451
452 \begin_layout Standard
453 A tree-level amplitude in 
454 \begin_inset Formula $e^{+}e^{-}$
455 \end_inset
456
457  collisions can be expressed in terms of fermion strings of the form 
458 \begin_inset Formula \begin{equation}
459 \bar{v}(p_{2},\sigma_{2})P_{-\tau}\hat{a}_{1}\hat{a}_{2}\cdots\hat{a}_{n}u(p_{1},\sigma_{1}),\end{equation}
460
461 \end_inset
462
463  where 
464 \begin_inset Formula $p$
465 \end_inset
466
467  and 
468 \begin_inset Formula $\sigma$
469 \end_inset
470
471  label the initial 
472 \begin_inset Formula $e^{\pm}$
473 \end_inset
474
475  four-momenta and helicities 
476 \begin_inset Formula $(\sigma=\pm1)$
477 \end_inset
478
479
480 \begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
481 \end_inset
482
483  and 
484 \begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
485 \end_inset
486
487  is a chirality projection operator 
488 \begin_inset Formula $(\tau=\pm1)$
489 \end_inset
490
491 .
492  The 
493 \begin_inset Formula $a_{i}^{\mu}$
494 \end_inset
495
496  may be formed from particle four-momenta, gauge-boson polarization vectors
497  or fermion strings with an uncontracted Lorentz index associated with final-sta
498 te fermions.
499 \end_layout
500
501 \begin_layout NoteToEditor
502 Figures 1 and 2 should appear side-by-side in print
503 \end_layout
504
505 \begin_layout Standard
506 In the chiral representation the 
507 \begin_inset Formula $\gamma$
508 \end_inset
509
510  matrices are expressed in terms of 
511 \begin_inset Formula $2\times2$
512 \end_inset
513
514  Pauli matrices 
515 \begin_inset Formula $\sigma$
516 \end_inset
517
518  and the unit matrix 1 as 
519 \begin_inset Formula \begin{eqnarray*}
520 \gamma^{\mu} & = & \left(\begin{array}{cc}
521 0 & \sigma_{+}^{\mu}\\
522 \sigma_{-}^{\mu} & 0\end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
523 -1 & 0\\
524 0 & 1\end{array}\right),\\
525 \sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),\end{eqnarray*}
526
527 \end_inset
528
529  giving 
530 \begin_inset Formula \begin{equation}
531 \hat{a}=\left(\begin{array}{cc}
532 0 & (\hat{a})_{+}\\
533 (\hat{a})_{-} & 0\end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},\end{equation}
534
535 \end_inset
536
537  The spinors are expressed in terms of two-component Weyl spinors as 
538 \begin_inset Formula \begin{equation}
539 u=\left(\begin{array}{c}
540 (u)_{-}\\
541 (u)_{+}\end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.\end{equation}
542
543 \end_inset
544
545
546 \end_layout
547
548 \begin_layout Standard
549 The Weyl spinors are given in terms of helicity eigenstates 
550 \begin_inset Formula $\chi_{\lambda}(p)$
551 \end_inset
552
553  with 
554 \begin_inset Formula $\lambda=\pm1$
555 \end_inset
556
557  by 
558 \end_layout
559
560 \begin_layout MathLetters
561 \begin_inset Formula \begin{eqnarray}
562 u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
563 v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)\end{eqnarray}
564
565 \end_inset
566
567
568 \end_layout
569
570 \begin_layout Section
571 Floating material and so forth
572 \end_layout
573
574 \begin_layout Standard
575 Consider a task that computes profile parameters for a modified Lorentzian
576  of the form 
577 \begin_inset Formula \begin{equation}
578 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}\end{equation}
579
580 \end_inset
581
582  where 
583 \begin_inset Formula \[
584 d_{1}=\sqrt{\left(\begin{array}{c}
585 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
586 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}\]
587
588 \end_inset
589
590
591 \begin_inset Formula \[
592 d_{2}=\sqrt{\left(\begin{array}{c}
593 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
594 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}\]
595
596 \end_inset
597
598
599 \begin_inset Formula \[
600 x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\]
601
602 \end_inset
603
604
605 \begin_inset Formula \[
606 y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta\]
607
608 \end_inset
609
610
611 \end_layout
612
613 \begin_layout Standard
614 In these expressions 
615 \begin_inset Formula $x_{0}$
616 \end_inset
617
618 ,
619 \begin_inset Formula $y_{0}$
620 \end_inset
621
622  is the star center, and 
623 \begin_inset Formula $\Theta$
624 \end_inset
625
626  is the angle with the 
627 \begin_inset Formula $x$
628 \end_inset
629
630  axis.
631  Results of this task are shown in table
632 \begin_inset space ~
633 \end_inset
634
635
636 \begin_inset CommandInset ref
637 LatexCommand ref
638 reference "tbl-2"
639
640 \end_inset
641
642 .
643  It is not clear how these sorts of analyses may affect determination of
644  
645 \begin_inset Formula $M_{\sun}$
646 \end_inset
647
648 , but the assumption is that the alternate results should be less than 90
649 \begin_inset ERT
650 status collapsed
651
652 \begin_layout Plain Layout
653
654
655 \backslash
656 degr
657 \backslash
658  
659 \end_layout
660
661 \end_inset
662
663 out of phase with previous values.
664  We have no observations of 
665 \begin_inset ERT
666 status collapsed
667
668 \begin_layout Plain Layout
669
670
671 \backslash
672 ion{Ca}{2}
673 \end_layout
674
675 \end_inset
676
677 .
678  Roughly 
679 \begin_inset ERT
680 status collapsed
681
682 \begin_layout Plain Layout
683
684
685 \backslash
686 slantfrac{4}{5}
687 \end_layout
688
689 \end_inset
690
691  of the electronically submitted abstracts for AAS meetings are error-free.
692 \end_layout
693
694 \begin_layout Acknowledgements
695
696 \end_layout
697
698 \begin_layout Standard
699 We are grateful to V.
700  Barger, T.
701  Han, and R.
702  J.
703  N.
704  Phillips for doing the math in section
705 \begin_inset space ~
706 \end_inset
707
708
709 \begin_inset CommandInset ref
710 LatexCommand ref
711 reference "bozomath"
712
713 \end_inset
714
715 .
716  More information on the AASTeX macros package are available at 
717 \begin_inset Flex URL
718 status collapsed
719
720 \begin_layout Plain Layout
721
722 http://www.aas.org/publications/aastex
723 \end_layout
724
725 \end_inset
726
727  or the 
728 \begin_inset ERT
729 status collapsed
730
731 \begin_layout Plain Layout
732
733
734 \backslash
735 anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
736 \end_layout
737
738 \end_inset
739
740 .
741 \end_layout
742
743 \begin_layout Appendix
744
745 \end_layout
746
747 \begin_layout Section
748 Appendicial material
749 \end_layout
750
751 \begin_layout Standard
752 Consider once again a task that computes profile parameters for a modified
753  Lorentzian of the form 
754 \begin_inset Formula \begin{equation}
755 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}\end{equation}
756
757 \end_inset
758
759  where 
760 \end_layout
761
762 \begin_layout MathLetters
763 \begin_inset Formula \[
764 d_{1}=\frac{3}{4}\sqrt{\left(\begin{array}{c}
765 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
766 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}\]
767
768 \end_inset
769
770
771 \begin_inset Formula \begin{equation}
772 d_{2}=\case{3}{4}\sqrt{\left(\begin{array}{c}
773 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
774 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}\end{equation}
775
776 \end_inset
777
778
779 \begin_inset Formula \begin{eqnarray}
780 x_{1} & = & (x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\\
781 y_{1} & = & -(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta\end{eqnarray}
782
783 \end_inset
784
785
786 \end_layout
787
788 \begin_layout Standard
789 For completeness, here is one last equation.
790  
791 \begin_inset Formula \begin{equation}
792 e=mc^{2}\end{equation}
793
794 \end_inset
795
796
797 \end_layout
798
799 \begin_layout References
800 \begin_inset CommandInset bibitem
801 LatexCommand bibitem
802 label "Auri\\`ere(1982)"
803 key "aur82"
804
805 \end_inset
806
807 Aurière, M.
808  1982, 
809 \begin_inset ERT
810 status collapsed
811
812 \begin_layout Plain Layout
813
814
815 \backslash
816 aap
817 \end_layout
818
819 \end_inset
820
821 , 109, 301 
822 \end_layout
823
824 \begin_layout References
825 \begin_inset CommandInset bibitem
826 LatexCommand bibitem
827 label "Canizares et al.(1978)"
828 key "can78"
829
830 \end_inset
831
832 Canizares, C.
833  R., Grindlay, J.
834  E., Hiltner, W.
835  A., Liller, W., and McClintock, J.
836  E.
837  1978, 
838 \begin_inset ERT
839 status collapsed
840
841 \begin_layout Plain Layout
842
843
844 \backslash
845 apj
846 \end_layout
847
848 \end_inset
849
850 , 224, 39 
851 \end_layout
852
853 \begin_layout References
854 \begin_inset CommandInset bibitem
855 LatexCommand bibitem
856 label "Djorgovski and King(1984)"
857 key "djo84"
858
859 \end_inset
860
861 Djorgovski, S., and King, I.
862  R.
863  1984, 
864 \begin_inset ERT
865 status collapsed
866
867 \begin_layout Plain Layout
868
869
870 \backslash
871 apjl
872 \end_layout
873
874 \end_inset
875
876 , 277, L49 
877 \end_layout
878
879 \begin_layout References
880 \begin_inset CommandInset bibitem
881 LatexCommand bibitem
882 label "Hagiwara and Zeppenfeld(1986)"
883 key "hag86"
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885 \end_inset
886
887 Hagiwara, K., and Zeppenfeld, D.
888  1986, Nucl.Phys., 274, 1 
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891 \begin_layout References
892 \begin_inset CommandInset bibitem
893 LatexCommand bibitem
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896
897 \end_inset
898
899 Harris, W.
900  E., and van den Bergh, S.
901  1984, 
902 \begin_inset ERT
903 status collapsed
904
905 \begin_layout Plain Layout
906
907
908 \backslash
909 aj
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911
912 \end_inset
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914 , 89, 1816 
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916
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924
925 Hénon, M.
926  1961, Ann.d'Ap., 24, 369 
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928
929 \begin_layout References
930 \begin_inset CommandInset bibitem
931 LatexCommand bibitem
932 label "King(1966)"
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934
935 \end_inset
936
937 King, I.
938  R.
939  1966, 
940 \begin_inset ERT
941 status collapsed
942
943 \begin_layout Plain Layout
944
945
946 \backslash
947 aj
948 \end_layout
949
950 \end_inset
951
952 , 71, 276 
953 \end_layout
954
955 \begin_layout References
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957 LatexCommand bibitem
958 label "King(1975)"
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960
961 \end_inset
962
963 King, I.
964  R.
965  1975, Dynamics of Stellar Systems, A.
966  Hayli, Dordrecht: Reidel, 1975, 99 
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969 \begin_layout References
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977 King, I.
978  R., Hedemann, E., Hodge, S.
979  M., and White, R.
980  E.
981  1968, 
982 \begin_inset ERT
983 status collapsed
984
985 \begin_layout Plain Layout
986
987
988 \backslash
989 aj
990 \end_layout
991
992 \end_inset
993
994 , 73, 456 
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996
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1002
1003 \end_inset
1004
1005 Kron, G.
1006  E., Hewitt, A.
1007  V., and Wasserman, L.
1008  H.
1009  1984, 
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1012
1013 \begin_layout Plain Layout
1014
1015
1016 \backslash
1017 pasp
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1019
1020 \end_inset
1021
1022 , 96, 198 
1023 \end_layout
1024
1025 \begin_layout References
1026 \begin_inset CommandInset bibitem
1027 LatexCommand bibitem
1028 label "Lynden-Bell and Wood(1968)"
1029 key "lyn68"
1030
1031 \end_inset
1032
1033 Lynden-Bell, D., and Wood, R.
1034  1968, 
1035 \begin_inset ERT
1036 status collapsed
1037
1038 \begin_layout Plain Layout
1039
1040
1041 \backslash
1042 mnras
1043 \end_layout
1044
1045 \end_inset
1046
1047 , 138, 495 
1048 \end_layout
1049
1050 \begin_layout References
1051 \begin_inset CommandInset bibitem
1052 LatexCommand bibitem
1053 label "Newell and O'Neil(1978)"
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1055
1056 \end_inset
1057
1058 Newell, E.
1059  B., and O'Neil, E.
1060  J.
1061  1978, 
1062 \begin_inset ERT
1063 status collapsed
1064
1065 \begin_layout Plain Layout
1066
1067
1068 \backslash
1069 apjs
1070 \end_layout
1071
1072 \end_inset
1073
1074 , 37, 27 
1075 \end_layout
1076
1077 \begin_layout References
1078 \begin_inset CommandInset bibitem
1079 LatexCommand bibitem
1080 label "Ortolani et al.(1985)"
1081 key "ort85"
1082
1083 \end_inset
1084
1085 Ortolani, S., Rosino, L., and Sandage, A.
1086  1985, 
1087 \begin_inset ERT
1088 status collapsed
1089
1090 \begin_layout Plain Layout
1091
1092
1093 \backslash
1094 aj
1095 \end_layout
1096
1097 \end_inset
1098
1099 , 90, 473 
1100 \end_layout
1101
1102 \begin_layout References
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1104 LatexCommand bibitem
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1106 key "pet76"
1107
1108 \end_inset
1109
1110 Peterson, C.
1111  J.
1112  1976, 
1113 \begin_inset ERT
1114 status collapsed
1115
1116 \begin_layout Plain Layout
1117
1118
1119 \backslash
1120 aj
1121 \end_layout
1122
1123 \end_inset
1124
1125 , 81, 617 
1126 \end_layout
1127
1128 \begin_layout References
1129 \begin_inset CommandInset bibitem
1130 LatexCommand bibitem
1131 label "Spitzer(1985)"
1132 key "spi85"
1133
1134 \end_inset
1135
1136 Spitzer, L.
1137  1985, Dynamics of Star Clusters, J.
1138  Goodman and P.
1139  Hut, Dordrecht: Reidel, 109 
1140 \end_layout
1141
1142 \begin_layout Standard
1143 \begin_inset ERT
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1145
1146 \begin_layout Plain Layout
1147
1148
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1150 clearpage
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1152
1153 \end_inset
1154
1155
1156 \end_layout
1157
1158 \begin_layout FigCaption
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1160 LatexCommand label
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1163 \end_inset
1164
1165 This is the first figure and it uses sgi9259.eps as its EPS figure file.
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1170 LatexCommand label
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1175 This is an example of a long figure caption that must be set as a paragraph.
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1178  
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1188 This figure has no associated EPS file, so the optional parameter is omitted.
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1199 \backslash
1200 clearpage
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1202
1203 \end_inset
1204
1205
1206 \end_layout
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1218 Terribly relevant tabular information.
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1220 LatexCommand label
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1223 \end_inset
1224
1225
1226 \end_layout
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1228 \end_inset
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1230
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1325
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1362 \begin_inset ERT
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1368 \backslash
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1371
1372 \end_inset
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1389
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1413 \begin_inset ERT
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1422
1423 \end_inset
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1425
1426 \end_layout
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1456
1457 \end_inset
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1459
1460 \end_layout
1461
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1767
1768 \begin_layout Plain Layout
1769 2.159 
1770 \end_layout
1771
1772 \end_inset
1773 </cell>
1774 <cell alignment="right" valignment="top" usebox="none">
1775 \begin_inset Text
1776
1777 \begin_layout Plain Layout
1778 6.7 
1779 \end_layout
1780
1781 \end_inset
1782 </cell>
1783 <cell alignment="right" valignment="top" usebox="none">
1784 \begin_inset Text
1785
1786 \begin_layout Plain Layout
1787 7.3 
1788 \end_layout
1789
1790 \end_inset
1791 </cell>
1792 <cell alignment="right" valignment="top" usebox="none">
1793 \begin_inset Text
1794
1795 \begin_layout Plain Layout
1796 -40.272
1797 \end_layout
1798
1799 \end_inset
1800 </cell>
1801 <cell alignment="right" valignment="top" usebox="none">
1802 \begin_inset Text
1803
1804 \begin_layout Plain Layout
1805 4
1806 \end_layout
1807
1808 \end_inset
1809 </cell>
1810 </row>
1811 <row>
1812 <cell alignment="center" valignment="top" usebox="none">
1813 \begin_inset Text
1814
1815 \begin_layout Plain Layout
1816  4 
1817 \end_layout
1818
1819 \end_inset
1820 </cell>
1821 <cell alignment="right" valignment="top" usebox="none">
1822 \begin_inset Text
1823
1824 \begin_layout Plain Layout
1825 32733.8 
1826 \end_layout
1827
1828 \end_inset
1829 </cell>
1830 <cell alignment="right" valignment="top" usebox="none">
1831 \begin_inset Text
1832
1833 \begin_layout Plain Layout
1834 -1.2
1835 \begin_inset ERT
1836 status collapsed
1837
1838 \begin_layout Plain Layout
1839
1840
1841 \backslash
1842 tablenotemark{c}
1843 \end_layout
1844
1845 \end_inset
1846
1847
1848 \end_layout
1849
1850 \end_inset
1851 </cell>
1852 <cell alignment="right" valignment="top" usebox="none">
1853 \begin_inset Text
1854
1855 \begin_layout Plain Layout
1856 -0.5 
1857 \end_layout
1858
1859 \end_inset
1860 </cell>
1861 <cell alignment="right" valignment="top" usebox="none">
1862 \begin_inset Text
1863
1864 \begin_layout Plain Layout
1865 41 
1866 \end_layout
1867
1868 \end_inset
1869 </cell>
1870 <cell alignment="right" valignment="top" usebox="none">
1871 \begin_inset Text
1872
1873 \begin_layout Plain Layout
1874 54.8 
1875 \end_layout
1876
1877 \end_inset
1878 </cell>
1879 <cell alignment="right" valignment="top" usebox="none">
1880 \begin_inset Text
1881
1882 \begin_layout Plain Layout
1883 2.282 
1884 \end_layout
1885
1886 \end_inset
1887 </cell>
1888 <cell alignment="right" valignment="top" usebox="none">
1889 \begin_inset Text
1890
1891 \begin_layout Plain Layout
1892 2.156 
1893 \end_layout
1894
1895 \end_inset
1896 </cell>
1897 <cell alignment="right" valignment="top" usebox="none">
1898 \begin_inset Text
1899
1900 \begin_layout Plain Layout
1901 4.313 
1902 \end_layout
1903
1904 \end_inset
1905 </cell>
1906 <cell alignment="right" valignment="top" usebox="none">
1907 \begin_inset Text
1908
1909 \begin_layout Plain Layout
1910 117.4 
1911 \end_layout
1912
1913 \end_inset
1914 </cell>
1915 <cell alignment="right" valignment="top" usebox="none">
1916 \begin_inset Text
1917
1918 \begin_layout Plain Layout
1919 78.2 
1920 \end_layout
1921
1922 \end_inset
1923 </cell>
1924 <cell alignment="right" valignment="top" usebox="none">
1925 \begin_inset Text
1926
1927 \begin_layout Plain Layout
1928 -35.847
1929 \end_layout
1930
1931 \end_inset
1932 </cell>
1933 <cell alignment="right" valignment="top" usebox="none">
1934 \begin_inset Text
1935
1936 \begin_layout Plain Layout
1937 5,6
1938 \end_layout
1939
1940 \end_inset
1941 </cell>
1942 </row>
1943 <row>
1944 <cell alignment="center" valignment="top" usebox="none">
1945 \begin_inset Text
1946
1947 \begin_layout Plain Layout
1948  5 
1949 \end_layout
1950
1951 \end_inset
1952 </cell>
1953 <cell alignment="right" valignment="top" usebox="none">
1954 \begin_inset Text
1955
1956 \begin_layout Plain Layout
1957  9607.4 
1958 \end_layout
1959
1960 \end_inset
1961 </cell>
1962 <cell alignment="right" valignment="top" usebox="none">
1963 \begin_inset Text
1964
1965 \begin_layout Plain Layout
1966 -0.4 
1967 \end_layout
1968
1969 \end_inset
1970 </cell>
1971 <cell alignment="right" valignment="top" usebox="none">
1972 \begin_inset Text
1973
1974 \begin_layout Plain Layout
1975 -0.4 
1976 \end_layout
1977
1978 \end_inset
1979 </cell>
1980 <cell alignment="right" valignment="top" usebox="none">
1981 \begin_inset Text
1982
1983 \begin_layout Plain Layout
1984 60 
1985 \end_layout
1986
1987 \end_inset
1988 </cell>
1989 <cell alignment="right" valignment="top" usebox="none">
1990 \begin_inset Text
1991
1992 \begin_layout Plain Layout
1993 1.4 
1994 \end_layout
1995
1996 \end_inset
1997 </cell>
1998 <cell alignment="right" valignment="top" usebox="none">
1999 \begin_inset Text
2000
2001 \begin_layout Plain Layout
2002 1.669
2003 \begin_inset ERT
2004 status collapsed
2005
2006 \begin_layout Plain Layout
2007
2008
2009 \backslash
2010 tablenotemark{c}
2011 \end_layout
2012
2013 \end_inset
2014
2015
2016 \end_layout
2017
2018 \end_inset
2019 </cell>
2020 <cell alignment="right" valignment="top" usebox="none">
2021 \begin_inset Text
2022
2023 \begin_layout Plain Layout
2024 1.574 
2025 \end_layout
2026
2027 \end_inset
2028 </cell>
2029 <cell alignment="right" valignment="top" usebox="none">
2030 \begin_inset Text
2031
2032 \begin_layout Plain Layout
2033 2.343 
2034 \end_layout
2035
2036 \end_inset
2037 </cell>
2038 <cell alignment="right" valignment="top" usebox="none">
2039 \begin_inset Text
2040
2041 \begin_layout Plain Layout
2042 8.0 
2043 \end_layout
2044
2045 \end_inset
2046 </cell>
2047 <cell alignment="right" valignment="top" usebox="none">
2048 \begin_inset Text
2049
2050 \begin_layout Plain Layout
2051 8.9 
2052 \end_layout
2053
2054 \end_inset
2055 </cell>
2056 <cell alignment="right" valignment="top" usebox="none">
2057 \begin_inset Text
2058
2059 \begin_layout Plain Layout
2060 -33.417
2061 \end_layout
2062
2063 \end_inset
2064 </cell>
2065 <cell alignment="right" valignment="top" usebox="none">
2066 \begin_inset Text
2067
2068 \begin_layout Plain Layout
2069 7
2070 \end_layout
2071
2072 \end_inset
2073 </cell>
2074 </row>
2075 <row>
2076 <cell alignment="center" valignment="top" usebox="none">
2077 \begin_inset Text
2078
2079 \begin_layout Plain Layout
2080  6 
2081 \end_layout
2082
2083 \end_inset
2084 </cell>
2085 <cell alignment="right" valignment="top" usebox="none">
2086 \begin_inset Text
2087
2088 \begin_layout Plain Layout
2089 31638.6 
2090 \end_layout
2091
2092 \end_inset
2093 </cell>
2094 <cell alignment="right" valignment="top" usebox="none">
2095 \begin_inset Text
2096
2097 \begin_layout Plain Layout
2098 1.6 
2099 \end_layout
2100
2101 \end_inset
2102 </cell>
2103 <cell alignment="right" valignment="top" usebox="none">
2104 \begin_inset Text
2105
2106 \begin_layout Plain Layout
2107 0.1 
2108 \end_layout
2109
2110 \end_inset
2111 </cell>
2112 <cell alignment="right" valignment="top" usebox="none">
2113 \begin_inset Text
2114
2115 \begin_layout Plain Layout
2116 39 
2117 \end_layout
2118
2119 \end_inset
2120 </cell>
2121 <cell alignment="right" valignment="top" usebox="none">
2122 \begin_inset Text
2123
2124 \begin_layout Plain Layout
2125 315.2 
2126 \end_layout
2127
2128 \end_inset
2129 </cell>
2130 <cell alignment="right" valignment="top" usebox="none">
2131 \begin_inset Text
2132
2133 \begin_layout Plain Layout
2134  3.433 
2135 \end_layout
2136
2137 \end_inset
2138 </cell>
2139 <cell alignment="right" valignment="top" usebox="none">
2140 \begin_inset Text
2141
2142 \begin_layout Plain Layout
2143 3.075 
2144 \end_layout
2145
2146 \end_inset
2147 </cell>
2148 <cell alignment="right" valignment="top" usebox="none">
2149 \begin_inset Text
2150
2151 \begin_layout Plain Layout
2152 7.488 
2153 \end_layout
2154
2155 \end_inset
2156 </cell>
2157 <cell alignment="right" valignment="top" usebox="none">
2158 \begin_inset Text
2159
2160 \begin_layout Plain Layout
2161 92.1 
2162 \end_layout
2163
2164 \end_inset
2165 </cell>
2166 <cell alignment="right" valignment="top" usebox="none">
2167 \begin_inset Text
2168
2169 \begin_layout Plain Layout
2170 25.3 
2171 \end_layout
2172
2173 \end_inset
2174 </cell>
2175 <cell alignment="right" valignment="top" usebox="none">
2176 \begin_inset Text
2177
2178 \begin_layout Plain Layout
2179 -12.052 
2180 \end_layout
2181
2182 \end_inset
2183 </cell>
2184 <cell alignment="right" valignment="top" usebox="none">
2185 \begin_inset Text
2186
2187 \begin_layout Plain Layout
2188 8
2189 \end_layout
2190
2191 \end_inset
2192 </cell>
2193 </row>
2194 </lyxtabular>
2195
2196 \end_inset
2197
2198
2199 \end_layout
2200
2201 \begin_layout Plain Layout
2202 \begin_inset ERT
2203 status collapsed
2204
2205 \begin_layout Plain Layout
2206
2207
2208 \backslash
2209 tablenotetext{a}{Sample footnote for table~
2210 \backslash
2211 ref{tbl-2} that was generated with the 
2212 \backslash
2213 LaTeX
2214 \backslash
2215  table environment} 
2216 \end_layout
2217
2218 \begin_layout Plain Layout
2219
2220 \end_layout
2221
2222 \begin_layout Plain Layout
2223
2224
2225 \backslash
2226 tablenotetext{b}{Yet another sample footnote for table~
2227 \backslash
2228 ref{tbl-2}} 
2229 \end_layout
2230
2231 \begin_layout Plain Layout
2232
2233 \end_layout
2234
2235 \begin_layout Plain Layout
2236
2237
2238 \backslash
2239 tablenotetext{c}{Another sample footnote for table~
2240 \backslash
2241 ref{tbl-2}}
2242 \end_layout
2243
2244 \end_inset
2245
2246
2247 \end_layout
2248
2249 \begin_layout TableComments
2250 We can also attach a long-ish paragraph of explanatory material to a table.
2251  Use 
2252 \backslash
2253 tablerefs to append a list of references.
2254  The following references were from a different table: I've patched them
2255  in here to show how they look, but don't take them too seriously---I certainly
2256  have not.
2257 \end_layout
2258
2259 \begin_layout TableRefs
2260 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
2261  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
2262  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
2263  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
2264  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
2265  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
2266  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
2267  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
2268  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
2269  al.
2270  1991; (26) Olsen 1983.
2271 \end_layout
2272
2273 \end_inset
2274
2275
2276 \end_layout
2277
2278 \begin_layout Standard
2279 \begin_inset ERT
2280 status collapsed
2281
2282 \begin_layout Plain Layout
2283
2284 % LyX can load deluxetable files verbatim.
2285  To see this in action, uncomment the following
2286 \end_layout
2287
2288 \end_inset
2289
2290
2291 \end_layout
2292
2293 \begin_layout Standard
2294 \begin_inset ERT
2295 status collapsed
2296
2297 \begin_layout Plain Layout
2298
2299 % line (delete the 
2300 \end_layout
2301
2302 \end_inset
2303
2304
2305 \begin_inset Quotes eld
2306 \end_inset
2307
2308
2309 \begin_inset ERT
2310 status collapsed
2311
2312 \begin_layout Plain Layout
2313
2314 %
2315 \end_layout
2316
2317 \end_inset
2318
2319
2320 \begin_inset Quotes erd
2321 \end_inset
2322
2323
2324 \begin_inset ERT
2325 status collapsed
2326
2327 \begin_layout Plain Layout
2328
2329 ) and copy the file table.tex from the AASTeX 5.0 distribution into
2330 \end_layout
2331
2332 \end_inset
2333
2334
2335 \end_layout
2336
2337 \begin_layout Standard
2338 \begin_inset ERT
2339 status collapsed
2340
2341 \begin_layout Plain Layout
2342
2343 % the same directory as this file.
2344 \end_layout
2345
2346 \end_inset
2347
2348
2349 \end_layout
2350
2351 \begin_layout Standard
2352 \begin_inset ERT
2353 status collapsed
2354
2355 \begin_layout Plain Layout
2356
2357 %
2358 \end_layout
2359
2360 \end_inset
2361
2362
2363 \begin_inset CommandInset include
2364 LatexCommand input
2365 filename "table"
2366
2367 \end_inset
2368
2369
2370 \end_layout
2371
2372 \end_body
2373 \end_document