lib/examples/aas_sample.lyx

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   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
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  66 \end_header
  67
  68 \begin_body
  69
  70 \begin_layout Title
  71 Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
  72  Examples
  73 \end_layout
  74
  75 \begin_layout Author
  76 S.
  77  Djorgovski
  78 \begin_inset Flex altaffilmark
  79 status open
  80
  81 \begin_layout Plain Layout
  82 1,2,3
  83 \end_layout
  84
  85 \end_inset
  86
  87  and Ivan R.
  88  King
  89 \begin_inset Flex altaffilmark
  90 status collapsed
  91
  92 \begin_layout Plain Layout
  93 1
  94 \end_layout
  95
  96 \end_inset
  97
  98
  99 \end_layout
 100
 101 \begin_layout Affiliation
 102 Astronomy Department, University of California, Berkeley, CA 94720
 103 \end_layout
 104
 105 \begin_layout Author
 106 C.
 107  D.
 108  Biemesderfer
 109 \begin_inset Flex altaffilmark
 110 status collapsed
 111
 112 \begin_layout Plain Layout
 113 4,5
 114 \end_layout
 115
 116 \end_inset
 117
 118
 119 \end_layout
 120
 121 \begin_layout Affiliation
 122 National Optical Astronomy Observatories, Tucson, AZ 85719
 123 \end_layout
 124
 125 \begin_layout Email
 126 aastex-help@aas.org
 127 \end_layout
 128
 129 \begin_layout And
 130
 131 \end_layout
 132
 133 \begin_layout Author
 134 R.
 135  J.
 136  Hanisch
 137 \begin_inset Flex altaffilmark
 138 status collapsed
 139
 140 \begin_layout Plain Layout
 141 5
 142 \end_layout
 143
 144 \end_inset
 145
 146
 147 \end_layout
 148
 149 \begin_layout Affiliation
 150 Space Telescope Science Institute, Baltimore, MD 21218
 151 \end_layout
 152
 153 \begin_layout Altaffilation
 154 1
 155 \begin_inset ERT
 156 status collapsed
 157
 158 \begin_layout Plain Layout
 159
 160 }{
 161 \end_layout
 162
 163 \end_inset
 164
 165 Visiting Astronomer, Cerro Tololo Inter-American Observatory.
 166  CTIO is operated by AURA, Inc.
 167 \begin_inset space \space{}
 168 \end_inset
 169
 170 under contract to the National Science Foundation.
 171 \end_layout
 172
 173 \begin_layout Altaffilation
 174 2
 175 \begin_inset ERT
 176 status collapsed
 177
 178 \begin_layout Plain Layout
 179
 180 }{
 181 \end_layout
 182
 183 \end_inset
 184
 185 Society of Fellows, Harvard University.
 186 \end_layout
 187
 188 \begin_layout Altaffilation
 189 3
 190 \begin_inset ERT
 191 status collapsed
 192
 193 \begin_layout Plain Layout
 194
 195 }{
 196 \end_layout
 197
 198 \end_inset
 199
 200 present address: Center for Astrophysics, 60 Garden Street, Cambridge, MA
 201  02138
 202 \end_layout
 203
 204 \begin_layout Altaffilation
 205 4
 206 \begin_inset ERT
 207 status collapsed
 208
 209 \begin_layout Plain Layout
 210
 211 }{
 212 \end_layout
 213
 214 \end_inset
 215
 216 Visiting Programmer, Space Telescope Science Institute
 217 \end_layout
 218
 219 \begin_layout Altaffilation
 220 5
 221 \begin_inset ERT
 222 status collapsed
 223
 224 \begin_layout Plain Layout
 225
 226 }{
 227 \end_layout
 228
 229 \end_inset
 230
 231 Patron, Alonso's Bar and Grill
 232 \end_layout
 233
 234 \begin_layout Abstract
 235 This is a preliminary report on surface photometry of the major fraction
 236  of known globular clusters, to see which of them show the signs of a collapsed
 237  core.
 238  We also explore some diversionary mathematics and recreational tables.
 239
 240 \end_layout
 241
 242 \begin_layout Keywords
 243 clusters: globular, peanut---bosons: bozos
 244 \end_layout
 245
 246 \begin_layout Section
 247 Introduction
 248 \end_layout
 249
 250 \begin_layout Standard
 251 A focal problem today in the dynamics of globular clusters is core collapse.
 252  It has been predicted by theory for decades
 253 \begin_inset ERT
 254 status collapsed
 255
 256 \begin_layout Plain Layout
 257
 258
 259 \backslash
 260 citep{hen61,lyn68,spi85}
 261 \end_layout
 262
 263 \end_inset
 264
 265 , but observation has been less alert to the phenomenon.
 266  For many years the central brightness peak in M15
 267 \begin_inset ERT
 268 status collapsed
 269
 270 \begin_layout Plain Layout
 271
 272
 273 \backslash
 274 citep{kin75,new78}
 275 \end_layout
 276
 277 \end_inset
 278
 279  seemed a unique anomaly.
 280  Then
 281 \begin_inset ERT
 282 status collapsed
 283
 284 \begin_layout Plain Layout
 285
 286
 287 \backslash
 288 citet{aur82}
 289 \end_layout
 290
 291 \end_inset
 292
 293  suggested a central peak in NGC 6397, and a limited photographic survey
 294  of ours
 295 \begin_inset ERT
 296 status collapsed
 297
 298 \begin_layout Plain Layout
 299
 300
 301 \backslash
 302 citep[Paper I]{djo84}
 303 \end_layout
 304
 305 \end_inset
 306
 307  found three more cases, including NGC 6624, whose sharp center had often
 308  been remarked on
 309 \begin_inset ERT
 310 status collapsed
 311
 312 \begin_layout Plain Layout
 313
 314
 315 \backslash
 316 citep{can78}
 317 \end_layout
 318
 319 \end_inset
 320
 321 .
 322
 323 \end_layout
 324
 325 \begin_layout Section
 326 Observations
 327 \end_layout
 328
 329 \begin_layout Standard
 330 All our observations were short direct exposures with CCD's.
 331  At Lick Observatory we used a TI 500
 332 \begin_inset Formula $\times$
 333 \end_inset
 334
 335 500 chip and a GEC 575
 336 \begin_inset Formula $\times$
 337 \end_inset
 338
 339 385, on the 1-m Nickel reflector.
 340  The only filter available at Lick was red.
 341  At CTIO we used a GEC 575
 342 \begin_inset Formula $\times$
 343 \end_inset
 344
 345 385, with
 346 \begin_inset Formula $B,V,$
 347 \end_inset
 348
 349  and
 350 \begin_inset Formula $R$
 351 \end_inset
 352
 353  filters, and an RCA 512
 354 \begin_inset Formula $\times$
 355 \end_inset
 356
 357 320, with
 358 \begin_inset Formula $U,B,V,R,$
 359 \end_inset
 360
 361  and
 362 \begin_inset Formula $I$
 363 \end_inset
 364
 365  filters, on the 1.5-m reflector.
 366  In the CTIO observations we tried to concentrate on the shortest practicable
 367  wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
 368  often kept us from observing in
 369 \begin_inset Formula $U$
 370 \end_inset
 371
 372  or even in
 373 \begin_inset Formula $B$
 374 \end_inset
 375
 376 .
 377  All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
 378  sizes were around 3 arcmin.
 379 \end_layout
 380
 381 \begin_layout Standard
 382 The CCD images are unfortunately not always suitable, for very poor clusters
 383  or for clusters with large cores.
 384  Since the latter are easily studied by other means, we augmented our own
 385  CCD profiles by collecting from the literature a number of star-count profiles
 386
 387 \begin_inset ERT
 388 status collapsed
 389
 390 \begin_layout Plain Layout
 391
 392
 393 \backslash
 394 citep{kin68,pet76,har84,ort85}
 395 \end_layout
 396
 397 \end_inset
 398
 399 , as well as photoelectric profiles
 400 \begin_inset ERT
 401 status collapsed
 402
 403 \begin_layout Plain Layout
 404
 405
 406 \backslash
 407 citep{kin66,kin75}
 408 \end_layout
 409
 410 \end_inset
 411
 412  and electronographic profiles
 413 \begin_inset ERT
 414 status collapsed
 415
 416 \begin_layout Plain Layout
 417
 418
 419 \backslash
 420 citep{kro84}
 421 \end_layout
 422
 423 \end_inset
 424
 425 .
 426  In a few cases we judged normality by eye estimates on one of the Sky Surveys.
 427 \end_layout
 428
 429 \begin_layout Section
 430 Helicity Amplitudes
 431 \end_layout
 432
 433 \begin_layout Standard
 434 It has been realized that helicity amplitudes provide a convenient means
 435  for Feynman diagram
 436 \begin_inset Foot
 437 status collapsed
 438
 439 \begin_layout Plain Layout
 440 Footnotes can be inserted like this.
 441 \end_layout
 442
 443 \end_inset
 444
 445  evaluations.
 446  These amplitude-level techniques are particularly convenient for calculations
 447  involving many Feynman diagrams, where the usual trace techniques for the
 448  amplitude squared becomes unwieldy.
 449  Our calculations use the helicity techniques developed by other authors
 450
 451 \begin_inset CommandInset citation
 452 LatexCommand cite
 453 key "hag86"
 454
 455 \end_inset
 456
 457 ; we briefly summarize below.
 458 \end_layout
 459
 460 \begin_layout Subsection
 461 Formalism
 462 \end_layout
 463
 464 \begin_layout Standard
 465 \begin_inset CommandInset label
 466 LatexCommand label
 467 name "bozomath"
 468
 469 \end_inset
 470
 471
 472 \end_layout
 473
 474 \begin_layout Standard
 475 A tree-level amplitude in
 476 \begin_inset Formula $e^{+}e^{-}$
 477 \end_inset
 478
 479  collisions can be expressed in terms of fermion strings of the form
 480 \begin_inset Formula
 481 \begin{equation}
 482 \bar{v}(p_{2},\sigma_{2})P_{-\tau}\hat{a}_{1}\hat{a}_{2}\cdots\hat{a}_{n}u(p_{1},\sigma_{1}),
 483 \end{equation}
 484
 485 \end_inset
 486
 487  where
 488 \begin_inset Formula $p$
 489 \end_inset
 490
 491  and
 492 \begin_inset Formula $\sigma$
 493 \end_inset
 494
 495  label the initial
 496 \begin_inset Formula $e^{\pm}$
 497 \end_inset
 498
 499  four-momenta and helicities
 500 \begin_inset Formula $(\sigma=\pm1)$
 501 \end_inset
 502
 503 ,
 504 \begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
 505 \end_inset
 506
 507  and
 508 \begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
 509 \end_inset
 510
 511  is a chirality projection operator
 512 \begin_inset Formula $(\tau=\pm1)$
 513 \end_inset
 514
 515 .
 516  The
 517 \begin_inset Formula $a_{i}^{\mu}$
 518 \end_inset
 519
 520  may be formed from particle four-momenta, gauge-boson polarization vectors
 521  or fermion strings with an uncontracted Lorentz index associated with final-sta
 522 te fermions.
 523 \end_layout
 524
 525 \begin_layout NoteToEditor
 526 Figures 1 and 2 should appear side-by-side in print
 527 \end_layout
 528
 529 \begin_layout Standard
 530 In the chiral representation the
 531 \begin_inset Formula $\gamma$
 532 \end_inset
 533
 534  matrices are expressed in terms of
 535 \begin_inset Formula $2\times2$
 536 \end_inset
 537
 538  Pauli matrices
 539 \begin_inset Formula $\sigma$
 540 \end_inset
 541
 542  and the unit matrix 1 as
 543 \begin_inset Formula
 544 \begin{eqnarray*}
 545 \gamma^{\mu} & = & \left(\begin{array}{cc}
 546 0 & \sigma_{+}^{\mu}\\
 547 \sigma_{-}^{\mu} & 0
 548 \end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
 549 -1 & 0\\
 550 0 & 1
 551 \end{array}\right),\\
 552 \sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),
 553 \end{eqnarray*}
 554
 555 \end_inset
 556
 557  giving
 558 \begin_inset Formula
 559 \begin{equation}
 560 \hat{a}=\left(\begin{array}{cc}
 561 0 & (\hat{a})_{+}\\
 562 (\hat{a})_{-} & 0
 563 \end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},
 564 \end{equation}
 565
 566 \end_inset
 567
 568  The spinors are expressed in terms of two-component Weyl spinors as
 569 \begin_inset Formula
 570 \begin{equation}
 571 u=\left(\begin{array}{c}
 572 (u)_{-}\\
 573 (u)_{+}
 574 \end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.
 575 \end{equation}
 576
 577 \end_inset
 578
 579
 580 \end_layout
 581
 582 \begin_layout Standard
 583 The Weyl spinors are given in terms of helicity eigenstates
 584 \begin_inset Formula $\chi_{\lambda}(p)$
 585 \end_inset
 586
 587  with
 588 \begin_inset Formula $\lambda=\pm1$
 589 \end_inset
 590
 591  by
 592 \end_layout
 593
 594 \begin_layout MathLetters
 595 \begin_inset Formula
 596 \begin{eqnarray}
 597 u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
 598 v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)
 599 \end{eqnarray}
 600
 601 \end_inset
 602
 603
 604 \end_layout
 605
 606 \begin_layout Section
 607 Floating material and so forth
 608 \end_layout
 609
 610 \begin_layout Standard
 611 Consider a task that computes profile parameters for a modified Lorentzian
 612  of the form
 613 \begin_inset Formula
 614 \begin{equation}
 615 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
 616 \end{equation}
 617
 618 \end_inset
 619
 620  where
 621 \begin_inset Formula
 622 \[
 623 d_{1}=\sqrt{\left(\begin{array}{c}
 624 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 625 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
 626 \]
 627
 628 \end_inset
 629
 630
 631 \begin_inset Formula
 632 \[
 633 d_{2}=\sqrt{\left(\begin{array}{c}
 634 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 635 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
 636 \]
 637
 638 \end_inset
 639
 640
 641 \begin_inset Formula
 642 \[
 643 x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta
 644 \]
 645
 646 \end_inset
 647
 648
 649 \begin_inset Formula
 650 \[
 651 y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
 652 \]
 653
 654 \end_inset
 655
 656
 657 \end_layout
 658
 659 \begin_layout Standard
 660 In these expressions
 661 \begin_inset Formula $x_{0}$
 662 \end_inset
 663
 664 ,
 665 \begin_inset Formula $y_{0}$
 666 \end_inset
 667
 668  is the star center, and
 669 \begin_inset Formula $\Theta$
 670 \end_inset
 671
 672  is the angle with the
 673 \begin_inset Formula $x$
 674 \end_inset
 675
 676  axis.
 677  Results of this task are shown in table
 678 \begin_inset space ~
 679 \end_inset
 680
 681
 682 \begin_inset CommandInset ref
 683 LatexCommand ref
 684 reference "tbl-2"
 685
 686 \end_inset
 687
 688 .
 689  It is not clear how these sorts of analyses may affect determination of
 690
 691 \begin_inset Formula $M_{\sun}$
 692 \end_inset
 693
 694 , but the assumption is that the alternate results should be less than 90°
 695  out of phase with previous values.
 696  We have no observations of
 697 \begin_inset ERT
 698 status collapsed
 699
 700 \begin_layout Plain Layout
 701
 702
 703 \backslash
 704 ion{Ca}{2}
 705 \end_layout
 706
 707 \end_inset
 708
 709 .
 710  Roughly
 711 \begin_inset ERT
 712 status collapsed
 713
 714 \begin_layout Plain Layout
 715
 716
 717 \backslash
 718 slantfrac{4}{5}
 719 \end_layout
 720
 721 \end_inset
 722
 723  of the electronically submitted abstracts for AAS meetings are error-free.
 724 \end_layout
 725
 726 \begin_layout Acknowledgements
 727
 728 \end_layout
 729
 730 \begin_layout Standard
 731 We are grateful to V.
 732  Barger, T.
 733  Han, and R.
 734  J.
 735  N.
 736  Phillips for doing the math in section
 737 \begin_inset space ~
 738 \end_inset
 739
 740
 741 \begin_inset CommandInset ref
 742 LatexCommand ref
 743 reference "bozomath"
 744
 745 \end_inset
 746
 747 .
 748  More information on the AASTeX macros package are available at
 749 \begin_inset Flex URL
 750 status collapsed
 751
 752 \begin_layout Plain Layout
 753
 754 http://www.aas.org/publications/aastex
 755 \end_layout
 756
 757 \end_inset
 758
 759  or the
 760 \begin_inset ERT
 761 status collapsed
 762
 763 \begin_layout Plain Layout
 764
 765
 766 \backslash
 767 anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
 768 \end_layout
 769
 770 \end_inset
 771
 772 .
 773 \end_layout
 774
 775 \begin_layout Appendix
 776
 777 \end_layout
 778
 779 \begin_layout Section
 780 Appendicial material
 781 \end_layout
 782
 783 \begin_layout Standard
 784 Consider once again a task that computes profile parameters for a modified
 785  Lorentzian of the form
 786 \begin_inset Formula
 787 \begin{equation}
 788 I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
 789 \end{equation}
 790
 791 \end_inset
 792
 793  where
 794 \end_layout
 795
 796 \begin_layout MathLetters
 797 \begin_inset Formula
 798 \[
 799 d_{1}=\frac{3}{4}\sqrt{\left(\begin{array}{c}
 800 \frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 801 \frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
 802 \]
 803
 804 \end_inset
 805
 806
 807 \begin_inset Formula
 808 \begin{equation}
 809 d_{2}=\case{3}{4}\sqrt{\left(\begin{array}{c}
 810 \frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
 811 \case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
 812 \end{equation}
 813
 814 \end_inset
 815
 816
 817 \begin_inset Formula
 818 \begin{eqnarray}
 819 x_{1} & = & (x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\\
 820 y_{1} & = & -(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
 821 \end{eqnarray}
 822
 823 \end_inset
 824
 825
 826 \end_layout
 827
 828 \begin_layout Standard
 829 For completeness, here is one last equation.
 830
 831 \begin_inset Formula
 832 \begin{equation}
 833 e=mc^{2}
 834 \end{equation}
 835
 836 \end_inset
 837
 838
 839 \end_layout
 840
 841 \begin_layout References
 842 \begin_inset CommandInset bibitem
 843 LatexCommand bibitem
 844 label "Auri\\`ere(1982)"
 845 key "aur82"
 846
 847 \end_inset
 848
 849 Aurière, M.
 850  1982,
 851 \begin_inset ERT
 852 status collapsed
 853
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1031 aj
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1059 pasp
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1061
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1086
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1108
1109
1110 \backslash
1111 apjs
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1113
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1127 Ortolani, S., Rosino, L., and Sandage, A.
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1130 status collapsed
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1136 aj
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1138
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1152 Peterson, C.
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1161 \backslash
1162 aj
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1164
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1169
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1172 LatexCommand bibitem
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1178 Spitzer, L.
1179  1985, Dynamics of Star Clusters, J.
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1744 \end_layout
1745
1746 \end_inset
1747 </cell>
1748 <cell alignment="right" valignment="top" usebox="none">
1749 \begin_inset Text
1750
1751 \begin_layout Plain Layout
1752 60
1753 \end_layout
1754
1755 \end_inset
1756 </cell>
1757 <cell alignment="right" valignment="top" usebox="none">
1758 \begin_inset Text
1759
1760 \begin_layout Plain Layout
1761 3.4
1762 \end_layout
1763
1764 \end_inset
1765 </cell>
1766 <cell alignment="right" valignment="top" usebox="none">
1767 \begin_inset Text
1768
1769 \begin_layout Plain Layout
1770 1.622
1771 \end_layout
1772
1773 \end_inset
1774 </cell>
1775 <cell alignment="right" valignment="top" usebox="none">
1776 \begin_inset Text
1777
1778 \begin_layout Plain Layout
1779 1.551
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 2.159
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 6.7
1798 \end_layout
1799
1800 \end_inset
1801 </cell>
1802 <cell alignment="right" valignment="top" usebox="none">
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1804
1805 \begin_layout Plain Layout
1806 7.3
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 -40.272
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1817
1818 \end_inset
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1820 <cell alignment="right" valignment="top" usebox="none">
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1822
1823 \begin_layout Plain Layout
1824 4
1825 \end_layout
1826
1827 \end_inset
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1829 </row>
1830 <row>
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1832 \begin_inset Text
1833
1834 \begin_layout Plain Layout
1835  4
1836 \end_layout
1837
1838 \end_inset
1839 </cell>
1840 <cell alignment="right" valignment="top" usebox="none">
1841 \begin_inset Text
1842
1843 \begin_layout Plain Layout
1844 32733.8
1845 \end_layout
1846
1847 \end_inset
1848 </cell>
1849 <cell alignment="right" valignment="top" usebox="none">
1850 \begin_inset Text
1851
1852 \begin_layout Plain Layout
1853 -1.2
1854 \begin_inset Flex tablenotemark
1855 status open
1856
1857 \begin_layout Plain Layout
1858 c
1859 \end_layout
1860
1861 \end_inset
1862
1863
1864 \end_layout
1865
1866 \end_inset
1867 </cell>
1868 <cell alignment="right" valignment="top" usebox="none">
1869 \begin_inset Text
1870
1871 \begin_layout Plain Layout
1872 -0.5
1873 \end_layout
1874
1875 \end_inset
1876 </cell>
1877 <cell alignment="right" valignment="top" usebox="none">
1878 \begin_inset Text
1879
1880 \begin_layout Plain Layout
1881 41
1882 \end_layout
1883
1884 \end_inset
1885 </cell>
1886 <cell alignment="right" valignment="top" usebox="none">
1887 \begin_inset Text
1888
1889 \begin_layout Plain Layout
1890 54.8
1891 \end_layout
1892
1893 \end_inset
1894 </cell>
1895 <cell alignment="right" valignment="top" usebox="none">
1896 \begin_inset Text
1897
1898 \begin_layout Plain Layout
1899 2.282
1900 \end_layout
1901
1902 \end_inset
1903 </cell>
1904 <cell alignment="right" valignment="top" usebox="none">
1905 \begin_inset Text
1906
1907 \begin_layout Plain Layout
1908 2.156
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 4.313
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 117.4
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 78.2
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 -35.847
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 5,6
1954 \end_layout
1955
1956 \end_inset
1957 </cell>
1958 </row>
1959 <row>
1960 <cell alignment="center" valignment="top" usebox="none">
1961 \begin_inset Text
1962
1963 \begin_layout Plain Layout
1964  5
1965 \end_layout
1966
1967 \end_inset
1968 </cell>
1969 <cell alignment="right" valignment="top" usebox="none">
1970 \begin_inset Text
1971
1972 \begin_layout Plain Layout
1973  9607.4
1974 \end_layout
1975
1976 \end_inset
1977 </cell>
1978 <cell alignment="right" valignment="top" usebox="none">
1979 \begin_inset Text
1980
1981 \begin_layout Plain Layout
1982 -0.4
1983 \end_layout
1984
1985 \end_inset
1986 </cell>
1987 <cell alignment="right" valignment="top" usebox="none">
1988 \begin_inset Text
1989
1990 \begin_layout Plain Layout
1991 -0.4
1992 \end_layout
1993
1994 \end_inset
1995 </cell>
1996 <cell alignment="right" valignment="top" usebox="none">
1997 \begin_inset Text
1998
1999 \begin_layout Plain Layout
2000 60
2001 \end_layout
2002
2003 \end_inset
2004 </cell>
2005 <cell alignment="right" valignment="top" usebox="none">
2006 \begin_inset Text
2007
2008 \begin_layout Plain Layout
2009 1.4
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 1.669
2019 \begin_inset Flex tablenotemark
2020 status collapsed
2021
2022 \begin_layout Plain Layout
2023 c
2024 \end_layout
2025
2026 \end_inset
2027
2028
2029 \end_layout
2030
2031 \end_inset
2032 </cell>
2033 <cell alignment="right" valignment="top" usebox="none">
2034 \begin_inset Text
2035
2036 \begin_layout Plain Layout
2037 1.574
2038 \end_layout
2039
2040 \end_inset
2041 </cell>
2042 <cell alignment="right" valignment="top" usebox="none">
2043 \begin_inset Text
2044
2045 \begin_layout Plain Layout
2046 2.343
2047 \end_layout
2048
2049 \end_inset
2050 </cell>
2051 <cell alignment="right" valignment="top" usebox="none">
2052 \begin_inset Text
2053
2054 \begin_layout Plain Layout
2055 8.0
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2057
2058 \end_inset
2059 </cell>
2060 <cell alignment="right" valignment="top" usebox="none">
2061 \begin_inset Text
2062
2063 \begin_layout Plain Layout
2064 8.9
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2066
2067 \end_inset
2068 </cell>
2069 <cell alignment="right" valignment="top" usebox="none">
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2071
2072 \begin_layout Plain Layout
2073 -33.417
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2075
2076 \end_inset
2077 </cell>
2078 <cell alignment="right" valignment="top" usebox="none">
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2080
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2082 7
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2087 </row>
2088 <row>
2089 <cell alignment="center" valignment="top" usebox="none">
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2091
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2097 </cell>
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2099 \begin_inset Text
2100
2101 \begin_layout Plain Layout
2102 31638.6
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2104
2105 \end_inset
2106 </cell>
2107 <cell alignment="right" valignment="top" usebox="none">
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2109
2110 \begin_layout Plain Layout
2111 1.6
2112 \end_layout
2113
2114 \end_inset
2115 </cell>
2116 <cell alignment="right" valignment="top" usebox="none">
2117 \begin_inset Text
2118
2119 \begin_layout Plain Layout
2120 0.1
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2122
2123 \end_inset
2124 </cell>
2125 <cell alignment="right" valignment="top" usebox="none">
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2127
2128 \begin_layout Plain Layout
2129 39
2130 \end_layout
2131
2132 \end_inset
2133 </cell>
2134 <cell alignment="right" valignment="top" usebox="none">
2135 \begin_inset Text
2136
2137 \begin_layout Plain Layout
2138 315.2
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  3.433
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 3.075
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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 7.488
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 92.1
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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 25.3
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 -12.052
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 8
2202 \end_layout
2203
2204 \end_inset
2205 </cell>
2206 </row>
2207 </lyxtabular>
2208
2209 \end_inset
2210
2211
2212 \end_layout
2213
2214 \begin_layout Table note
2215 a
2216 \begin_inset ERT
2217 status collapsed
2218
2219 \begin_layout Plain Layout
2220
2221 }{
2222 \end_layout
2223
2224 \end_inset
2225
2226 Sample footnote for table
2227 \begin_inset space ~
2228 \end_inset
2229
2230
2231 \begin_inset CommandInset ref
2232 LatexCommand ref
2233 reference "tbl-2"
2234
2235 \end_inset
2236
2237  that was generated with the LaTeX table environment
2238 \end_layout
2239
2240 \begin_layout Table note
2241 b
2242 \begin_inset ERT
2243 status collapsed
2244
2245 \begin_layout Plain Layout
2246
2247 }{
2248 \end_layout
2249
2250 \end_inset
2251
2252 Yet another sample footnote for table
2253 \begin_inset space ~
2254 \end_inset
2255
2256
2257 \begin_inset CommandInset ref
2258 LatexCommand ref
2259 reference "tbl-2"
2260
2261 \end_inset
2262
2263
2264 \end_layout
2265
2266 \begin_layout Table note
2267 c
2268 \begin_inset ERT
2269 status collapsed
2270
2271 \begin_layout Plain Layout
2272
2273 }{
2274 \end_layout
2275
2276 \end_inset
2277
2278 Another sample footnote for table
2279 \begin_inset space ~
2280 \end_inset
2281
2282
2283 \begin_inset CommandInset ref
2284 LatexCommand ref
2285 reference "tbl-2"
2286
2287 \end_inset
2288
2289
2290 \end_layout
2291
2292 \begin_layout TableComments
2293 We can also attach a long-ish paragraph of explanatory material to a table.
2294  Use
2295 \backslash
2296 tablerefs to append a list of references.
2297  The following references were from a different table: I've patched them
2298  in here to show how they look, but don't take them too seriously---I certainly
2299  have not.
2300 \end_layout
2301
2302 \begin_layout TableRefs
2303 (1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
2304  1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
2305  1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
2306  & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
2307  1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
2308  & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
2309  (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
2310  Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
2311  1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
2312  al.
2313  1991; (26) Olsen 1983.
2314 \end_layout
2315
2316 \end_inset
2317
2318
2319 \end_layout
2320
2321 \begin_layout Standard
2322 \begin_inset ERT
2323 status collapsed
2324
2325 \begin_layout Plain Layout
2326
2327 % LyX can load deluxetable files verbatim.
2328  To see this in action, uncomment the following
2329 \end_layout
2330
2331 \end_inset
2332
2333
2334 \end_layout
2335
2336 \begin_layout Standard
2337 \begin_inset ERT
2338 status collapsed
2339
2340 \begin_layout Plain Layout
2341
2342 % line (delete the
2343 \end_layout
2344
2345 \end_inset
2346
2347
2348 \begin_inset Quotes eld
2349 \end_inset
2350
2351
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 Quotes erd
2364 \end_inset
2365
2366
2367 \begin_inset ERT
2368 status collapsed
2369
2370 \begin_layout Plain Layout
2371
2372 ) and copy the file table.tex from the AASTeX 5.0 distribution into
2373 \end_layout
2374
2375 \end_inset
2376
2377
2378 \end_layout
2379
2380 \begin_layout Standard
2381 \begin_inset ERT
2382 status collapsed
2383
2384 \begin_layout Plain Layout
2385
2386 % the same directory as this file.
2387 \end_layout
2388
2389 \end_inset
2390
2391
2392 \end_layout
2393
2394 \begin_layout Standard
2395 \begin_inset ERT
2396 status collapsed
2397
2398 \begin_layout Plain Layout
2399
2400 %
2401 \end_layout
2402
2403 \end_inset
2404
2405
2406 \begin_inset CommandInset include
2407 LatexCommand input
2408 filename "table"
2409
2410 \end_inset
2411
2412
2413 \end_layout
2414
2415 \end_body
2416 \end_document