--- /dev/null
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+\lyxformat 507
+\begin_document
+\begin_header
+\save_transient_properties true
+\origin /systemlyxdir/examples/
+\textclass aastex
+\begin_preamble
+\newcommand{\vdag}{(v)^\dagger}
+\newcommand{\myemail}{skywalker@galaxy.far.far.away}
+\slugcomment{Not to appear in Nonlearned J., 45.}
+\shorttitle{Djorgovski et al.}
+\shortauthors{Collapsed Cores in Globular Clusters}
+\end_preamble
+\use_default_options false
+\maintain_unincluded_children false
+\language english
+\language_package default
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+\use_package stackrel 0
+\use_package stmaryrd 0
+\use_package undertilde 0
+\cite_engine basic
+\cite_engine_type default
+\biblio_style plain
+\use_bibtopic false
+\use_indices false
+\paperorientation portrait
+\suppress_date false
+\justification true
+\use_refstyle 0
+\index Index
+\shortcut idx
+\color #008000
+\end_index
+\secnumdepth 3
+\tocdepth 3
+\paragraph_separation indent
+\paragraph_indentation default
+\quotes_language english
+\papercolumns 1
+\papersides 1
+\paperpagestyle default
+\tracking_changes false
+\html_math_output 0
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+\output_changes false
+\html_be_strict false
+\end_header
+
+\begin_body
+
+\begin_layout Title
+Collapsed Cores in Globular Clusters, Gauge-Boson Couplings, and AAS\SpecialChar TeX
+ Examples
+\end_layout
+
+\begin_layout Author
+S.
+ Djorgovski
+\begin_inset Flex altaffilmark
+status open
+
+\begin_layout Plain Layout
+1,2,3
+\end_layout
+
+\end_inset
+
+ and Ivan R.
+ King
+\begin_inset Flex altaffilmark
+status collapsed
+
+\begin_layout Plain Layout
+1
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Affiliation
+Astronomy Department, University of California, Berkeley, CA 94720
+\end_layout
+
+\begin_layout Author
+C.
+ D.
+ Biemesderfer
+\begin_inset Flex altaffilmark
+status collapsed
+
+\begin_layout Plain Layout
+4,5
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Affiliation
+National Optical Astronomy Observatories, Tucson, AZ 85719
+\end_layout
+
+\begin_layout Email
+aastex-help@aas.org
+\end_layout
+
+\begin_layout And
+
+\end_layout
+
+\begin_layout Author
+R.
+ J.
+ Hanisch
+\begin_inset Flex altaffilmark
+status collapsed
+
+\begin_layout Plain Layout
+5
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Affiliation
+Space Telescope Science Institute, Baltimore, MD 21218
+\end_layout
+
+\begin_layout Altaffilation
+\begin_inset Argument 1
+status open
+
+\begin_layout Plain Layout
+1
+\end_layout
+
+\end_inset
+
+Visiting Astronomer, Cerro Tololo Inter-American Observatory.
+ CTIO is operated by AURA, Inc.
+\begin_inset space \space{}
+\end_inset
+
+under contract to the National Science Foundation.
+\end_layout
+
+\begin_layout Altaffilation
+\begin_inset Argument 1
+status open
+
+\begin_layout Plain Layout
+2
+\end_layout
+
+\end_inset
+
+Society of Fellows, Harvard University.
+\end_layout
+
+\begin_layout Altaffilation
+\begin_inset Argument 1
+status open
+
+\begin_layout Plain Layout
+3
+\end_layout
+
+\end_inset
+
+present address: Center for Astrophysics, 60 Garden Street, Cambridge, MA
+ 02138
+\end_layout
+
+\begin_layout Altaffilation
+\begin_inset Argument 1
+status open
+
+\begin_layout Plain Layout
+4
+\end_layout
+
+\end_inset
+
+Visiting Programmer, Space Telescope Science Institute
+\end_layout
+
+\begin_layout Altaffilation
+\begin_inset Argument 1
+status open
+
+\begin_layout Plain Layout
+5
+\end_layout
+
+\end_inset
+
+Patron, Alonso's Bar and Grill
+\end_layout
+
+\begin_layout Abstract
+This is a preliminary report on surface photometry of the major fraction
+ of known globular clusters, to see which of them show the signs of a collapsed
+ core.
+ We also explore some diversionary mathematics and recreational tables.
+
+\end_layout
+
+\begin_layout Keywords
+clusters: globular, peanut—bosons: bozos
+\end_layout
+
+\begin_layout Section
+Introduction
+\end_layout
+
+\begin_layout Standard
+A focal problem today in the dynamics of globular clusters is core collapse.
+ It has been predicted by theory for decades
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep{hen61,lyn68,spi85}
+\end_layout
+
+\end_inset
+
+, but observation has been less alert to the phenomenon.
+ For many years the central brightness peak in M15
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep{kin75,new78}
+\end_layout
+
+\end_inset
+
+ seemed a unique anomaly.
+ Then
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citet{aur82}
+\end_layout
+
+\end_inset
+
+ suggested a central peak in NGC 6397, and a limited photographic survey
+ of ours
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep[Paper I]{djo84}
+\end_layout
+
+\end_inset
+
+ found three more cases, including NGC 6624, whose sharp center had often
+ been remarked on
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep{can78}
+\end_layout
+
+\end_inset
+
+.
+
+\end_layout
+
+\begin_layout Section
+Observations
+\end_layout
+
+\begin_layout Standard
+All our observations were short direct exposures with CCD's.
+ At Lick Observatory we used a TI 500
+\begin_inset Formula $\times$
+\end_inset
+
+500 chip and a GEC 575
+\begin_inset Formula $\times$
+\end_inset
+
+385, on the 1-m Nickel reflector.
+ The only filter available at Lick was red.
+ At CTIO we used a GEC 575
+\begin_inset Formula $\times$
+\end_inset
+
+385, with
+\begin_inset Formula $B,V,$
+\end_inset
+
+ and
+\begin_inset Formula $R$
+\end_inset
+
+ filters, and an RCA 512
+\begin_inset Formula $\times$
+\end_inset
+
+320, with
+\begin_inset Formula $U,B,V,R,$
+\end_inset
+
+ and
+\begin_inset Formula $I$
+\end_inset
+
+ filters, on the 1.5-m reflector.
+ In the CTIO observations we tried to concentrate on the shortest practicable
+ wavelengths; but faintness, reddening, and poor short-wavelength sensitivity
+ often kept us from observing in
+\begin_inset Formula $U$
+\end_inset
+
+ or even in
+\begin_inset Formula $B$
+\end_inset
+
+.
+ All four cameras had scales of the order of 0.4 arcsec/pixel, and our field
+ sizes were around 3 arcmin.
+\end_layout
+
+\begin_layout Standard
+The CCD images are unfortunately not always suitable, for very poor clusters
+ or for clusters with large cores.
+ Since the latter are easily studied by other means, we augmented our own
+ CCD profiles by collecting from the literature a number of star-count profiles
+
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep{kin68,pet76,har84,ort85}
+\end_layout
+
+\end_inset
+
+, as well as photoelectric profiles
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep{kin66,kin75}
+\end_layout
+
+\end_inset
+
+ and electronographic profiles
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+citep{kro84}
+\end_layout
+
+\end_inset
+
+.
+ In a few cases we judged normality by eye estimates on one of the Sky Surveys.
+\end_layout
+
+\begin_layout Section
+Helicity Amplitudes
+\end_layout
+
+\begin_layout Standard
+It has been realized that helicity amplitudes provide a convenient means
+ for Feynman diagram
+\begin_inset Foot
+status collapsed
+
+\begin_layout Plain Layout
+Footnotes can be inserted like this.
+\end_layout
+
+\end_inset
+
+ evaluations.
+ These amplitude-level techniques are particularly convenient for calculations
+ involving many Feynman diagrams, where the usual trace techniques for the
+ amplitude squared becomes unwieldy.
+ Our calculations use the helicity techniques developed by other authors
+
+\begin_inset CommandInset citation
+LatexCommand cite
+key "hag86"
+
+\end_inset
+
+; we briefly summarize below.
+\end_layout
+
+\begin_layout Subsection
+Formalism
+\end_layout
+
+\begin_layout Standard
+\begin_inset CommandInset label
+LatexCommand label
+name "bozomath"
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+A tree-level amplitude in
+\begin_inset Formula $e^{+}e^{-}$
+\end_inset
+
+ collisions can be expressed in terms of fermion strings of the form
+\begin_inset Formula
+\begin{equation}
+\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}
+
+\end_inset
+
+ where
+\begin_inset Formula $p$
+\end_inset
+
+ and
+\begin_inset Formula $\sigma$
+\end_inset
+
+ label the initial
+\begin_inset Formula $e^{\pm}$
+\end_inset
+
+ four-momenta and helicities
+\begin_inset Formula $(\sigma=\pm1)$
+\end_inset
+
+,
+\begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$
+\end_inset
+
+ and
+\begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$
+\end_inset
+
+ is a chirality projection operator
+\begin_inset Formula $(\tau=\pm1)$
+\end_inset
+
+.
+ The
+\begin_inset Formula $a_{i}^{\mu}$
+\end_inset
+
+ may be formed from particle four-momenta, gauge-boson polarization vectors
+ or fermion strings with an uncontracted Lorentz index associated with final-sta
+te fermions.
+\end_layout
+
+\begin_layout NoteToEditor
+Figures 1 and 2 should appear side-by-side in print
+\end_layout
+
+\begin_layout Standard
+In the chiral representation the
+\begin_inset Formula $\gamma$
+\end_inset
+
+ matrices are expressed in terms of
+\begin_inset Formula $2\times2$
+\end_inset
+
+ Pauli matrices
+\begin_inset Formula $\sigma$
+\end_inset
+
+ and the unit matrix 1 as
+\begin_inset Formula
+\begin{eqnarray*}
+\gamma^{\mu} & = & \left(\begin{array}{cc}
+0 & \sigma_{+}^{\mu}\\
+\sigma_{-}^{\mu} & 0
+\end{array}\right),\gamma^{5}=\left(\begin{array}{cc}
+-1 & 0\\
+0 & 1
+\end{array}\right),\\
+\sigma_{\pm}^{\mu} & = & ({\textbf{1}},\pm\sigma),
+\end{eqnarray*}
+
+\end_inset
+
+ giving
+\begin_inset Formula
+\begin{equation}
+\hat{a}=\left(\begin{array}{cc}
+0 & (\hat{a})_{+}\\
+(\hat{a})_{-} & 0
+\end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu},
+\end{equation}
+
+\end_inset
+
+ The spinors are expressed in terms of two-component Weyl spinors as
+\begin_inset Formula
+\begin{equation}
+u=\left(\begin{array}{c}
+(u)_{-}\\
+(u)_{+}
+\end{array}\right),v={\textbf{(}}\vdag_{+}{\textbf{,}}\vdag_{-}{\textbf{)}}.
+\end{equation}
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+The Weyl spinors are given in terms of helicity eigenstates
+\begin_inset Formula $\chi_{\lambda}(p)$
+\end_inset
+
+ with
+\begin_inset Formula $\lambda=\pm1$
+\end_inset
+
+ by
+\end_layout
+
+\begin_layout MathLetters
+\begin_inset Formula
+\begin{eqnarray}
+u(p,\lambda)_{\pm} & = & (E\pm\lambda|{\textbf{p}}|)^{1/2}\chi_{\lambda}(p),\\
+v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|{\textbf{p}}|)^{1/2}\chi_{-\lambda}(p)
+\end{eqnarray}
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Section
+Floating material and so forth
+\end_layout
+
+\begin_layout Standard
+Consider a task that computes profile parameters for a modified Lorentzian
+ of the form
+\begin_inset Formula
+\begin{equation}
+I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
+\end{equation}
+
+\end_inset
+
+ where
+\begin_inset Formula
+\[
+d_{1}=\sqrt{\left(\begin{array}{c}
+\frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
+\frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
+\]
+
+\end_inset
+
+
+\begin_inset Formula
+\[
+d_{2}=\sqrt{\left(\begin{array}{c}
+\frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
+\case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
+\]
+
+\end_inset
+
+
+\begin_inset Formula
+\[
+x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta
+\]
+
+\end_inset
+
+
+\begin_inset Formula
+\[
+y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
+\]
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+In these expressions
+\begin_inset Formula $x_{0}$
+\end_inset
+
+,
+\begin_inset Formula $y_{0}$
+\end_inset
+
+ is the star center, and
+\begin_inset Formula $\Theta$
+\end_inset
+
+ is the angle with the
+\begin_inset Formula $x$
+\end_inset
+
+ axis.
+ Results of this task are shown in table
+\begin_inset space ~
+\end_inset
+
+
+\begin_inset CommandInset ref
+LatexCommand ref
+reference "tbl-2"
+
+\end_inset
+
+.
+ It is not clear how these sorts of analyses may affect determination of
+
+\begin_inset Formula $M_{\sun}$
+\end_inset
+
+, but the assumption is that the alternate results should be less than 90°
+ out of phase with previous values.
+ We have no observations of
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+ion{Ca}{2}
+\end_layout
+
+\end_inset
+
+.
+ Roughly
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+slantfrac{4}{5}
+\end_layout
+
+\end_inset
+
+ of the electronically submitted abstracts for AAS meetings are error-free.
+\end_layout
+
+\begin_layout Acknowledgements
+
+\end_layout
+
+\begin_layout Standard
+We are grateful to V.
+ Barger, T.
+ Han, and R.
+ J.
+ N.
+ Phillips for doing the math in section
+\begin_inset space ~
+\end_inset
+
+
+\begin_inset CommandInset ref
+LatexCommand ref
+reference "bozomath"
+
+\end_inset
+
+.
+ More information on the AAS\SpecialChar TeX
+ macros package are available at
+\begin_inset Flex URL
+status collapsed
+
+\begin_layout Plain Layout
+
+http://www.aas.org/publications/aastex
+\end_layout
+
+\end_inset
+
+ or the
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+anchor{
+\end_layout
+
+\end_inset
+
+ftp://www.aas.org/pubs/
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+}{
+\end_layout
+
+\end_inset
+
+AAS ftp site
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+}
+\end_layout
+
+\end_inset
+
+.
+\end_layout
+
+\begin_layout Appendix
+
+\end_layout
+
+\begin_layout Section
+Appendicial material
+\end_layout
+
+\begin_layout Standard
+Consider once again a task that computes profile parameters for a modified
+ Lorentzian of the form
+\begin_inset Formula
+\begin{equation}
+I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
+\end{equation}
+
+\end_inset
+
+ where
+\end_layout
+
+\begin_layout MathLetters
+\begin_inset Formula
+\[
+d_{1}=\frac{3}{4}\sqrt{\left(\begin{array}{c}
+\frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
+\frac{y_{1}}{R_{min}}\end{array}\right)^{2}}
+\]
+
+\end_inset
+
+
+\begin_inset Formula
+\begin{equation}
+d_{2}=\case{3}{4}\sqrt{\left(\begin{array}{c}
+\frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c}
+\case{y_{1}}{PR_{min}}\end{array}\right)^{2}}
+\end{equation}
+
+\end_inset
+
+
+\begin_inset Formula
+\begin{eqnarray}
+x_{1} & = & (x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta\\
+y_{1} & = & -(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta
+\end{eqnarray}
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+For completeness, here is one last equation.
+
+\begin_inset Formula
+\begin{equation}
+e=mc^{2}
+\end{equation}
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Auri\\`ere(1982)"
+key "aur82"
+
+\end_inset
+
+Aurière, M.
+ 1982,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+aap
+\end_layout
+
+\end_inset
+
+, 109, 301
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Canizares et al.(1978)"
+key "can78"
+
+\end_inset
+
+Canizares, C.
+ R., Grindlay, J.
+ E., Hiltner, W.
+ A., Liller, W., and McClintock, J.
+ E.
+ 1978,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+apj
+\end_layout
+
+\end_inset
+
+, 224, 39
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Djorgovski and King(1984)"
+key "djo84"
+
+\end_inset
+
+Djorgovski, S., and King, I.
+ R.
+ 1984,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+apjl
+\end_layout
+
+\end_inset
+
+, 277, L49
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Hagiwara and Zeppenfeld(1986)"
+key "hag86"
+
+\end_inset
+
+Hagiwara, K., and Zeppenfeld, D.
+ 1986, Nucl.Phys., 274, 1
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Harris and van den Bergh(1984)"
+key "har84"
+
+\end_inset
+
+Harris, W.
+ E., and van den Bergh, S.
+ 1984,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+aj
+\end_layout
+
+\end_inset
+
+, 89, 1816
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "H\\`enon(1961)"
+key "hen61"
+
+\end_inset
+
+Hénon, M.
+ 1961, Ann.d'Ap., 24, 369
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "King(1966)"
+key "kin66"
+
+\end_inset
+
+King, I.
+ R.
+ 1966,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+aj
+\end_layout
+
+\end_inset
+
+, 71, 276
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "King(1975)"
+key "kin75"
+
+\end_inset
+
+King, I.
+ R.
+ 1975, Dynamics of Stellar Systems, A.
+ Hayli, Dordrecht: Reidel, 1975, 99
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "King et al.(1968)"
+key "kin68"
+
+\end_inset
+
+King, I.
+ R., Hedemann, E., Hodge, S.
+ M., and White, R.
+ E.
+ 1968,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+aj
+\end_layout
+
+\end_inset
+
+, 73, 456
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Kron et al.(1984)"
+key "kro84"
+
+\end_inset
+
+Kron, G.
+ E., Hewitt, A.
+ V., and Wasserman, L.
+ H.
+ 1984,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+pasp
+\end_layout
+
+\end_inset
+
+, 96, 198
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Lynden-Bell and Wood(1968)"
+key "lyn68"
+
+\end_inset
+
+Lynden-Bell, D., and Wood, R.
+ 1968,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+mnras
+\end_layout
+
+\end_inset
+
+, 138, 495
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Newell and O'Neil(1978)"
+key "new78"
+
+\end_inset
+
+Newell, E.
+ B., and O'Neil, E.
+ J.
+ 1978,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+apjs
+\end_layout
+
+\end_inset
+
+, 37, 27
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
+label "Ortolani et al.(1985)"
+key "ort85"
+
+\end_inset
+
+Ortolani, S., Rosino, L., and Sandage, A.
+ 1985,
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+
+\backslash
+aj
+\end_layout
+
+\end_inset
+
+, 90, 473
+\end_layout
+
+\begin_layout References
+\begin_inset CommandInset bibitem
+LatexCommand bibitem
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+\end_inset
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+\begin_layout TableComments
+We can also attach a long-ish paragraph of explanatory material to a table.
+ Use
+\backslash
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+ The following references were from a different table: I've patched them
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+ have not.
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+
+\begin_layout TableRefs
+(1) Barbuy, Spite, & Spite 1985; (2) Bond 1980; (3) Carbon et al.
+ 1987; (4) Hobbs & Duncan 1987; (5) Gilroy et al.
+ 1988: (6) Gratton & Ortolani 1986; (7) Gratton & Sneden 1987; (8) Gratton
+ & Sneden (1988); (9) Gratton & Sneden 1991; (10) Kraft et al.
+ 1982; (11) LCL, or Laird, 1990; (12) Leep & Wallerstein 1981; (13) Luck
+ & Bond 1981; (14) Luck & Bond 1985; (15) Magain 1987; (16) Magain 1989;
+ (17) Peterson 1981; (18) Peterson, Kurucz, & Carney 1990; (19) RMB; (20)
+ Schuster & Nissen 1988; (21) Schuster & Nissen 1989b; (22) Spite et al.
+ 1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
+ al.
+ 1991; (26) Olsen 1983.
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+% LyX can load deluxetable files verbatim.
+ To see this in action, uncomment the following
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+% line (delete the
+\end_layout
+
+\end_inset
+
+
+\begin_inset Quotes eld
+\end_inset
+
+
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+%
+\end_layout
+
+\end_inset
+
+
+\begin_inset Quotes erd
+\end_inset
+
+
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+) and copy the file table.tex from the AASTeX 5.0 distribution into
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+% the same directory as this file.
+\end_layout
+
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+\begin_inset ERT
+status collapsed
+
+\begin_layout Plain Layout
+
+%
+\end_layout
+
+\end_inset
+
+
+\begin_inset CommandInset include
+LatexCommand input
+filename "table"
+
+\end_inset
+
+
+\end_layout
+
+\end_body
+\end_document
projects / lyx.git / commitdiff