lyx_mirror/lib/examples/aas_sample.lyx

#LyX 1.4.0cvs created this file. For more info see http://www.lyx.org/
\lyxformat 243
\begin_document
\begin_header
\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
\language english
\inputencoding default
\fontscheme default
\graphics default
\paperfontsize default
\spacing single
\papersize default
\use_geometry false
\use_amsmath 0
\cite_engine basic
\use_bibtopic false
\paperorientation portrait
\secnumdepth 3
\tocdepth 3
\paragraph_separation indent
\defskip medskip
\quotes_language english
\quotes_times 2
\papercolumns 1
\papersides 1
\paperpagestyle default
\tracking_changes false
\output_changes true
\end_header

\begin_body

\begin_layout Title

Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX 
Examples
\end_layout

\begin_layout Author

S.
 Djorgovski
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
altaffilmark{1,2,3}
\end_layout

\end_inset

 and Ivan R.
 King
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
altaffilmark{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 ERT
status collapsed

\begin_layout Standard

\backslash
altaffilmark{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 ERT
status collapsed

\begin_layout Standard

\backslash
altaffilmark{5}
\end_layout

\end_inset


\end_layout

\begin_layout Affiliation

Space Telescope Science Institute, Baltimore, MD 21218
\end_layout

\begin_layout Standard


\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
 CTIO is operated by AURA, Inc.
\backslash
 under contract to the National Science Foundation.} 
\end_layout

\begin_layout Standard

\end_layout

\begin_layout Standard

\backslash
altaffiltext{2}{Society of Fellows, Harvard University.} 
\end_layout

\begin_layout Standard

\end_layout

\begin_layout Standard

\backslash
altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
 Cambridge, MA 02138} 
\end_layout

\begin_layout Standard

\end_layout

\begin_layout Standard

\backslash
altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
 
\end_layout

\begin_layout Standard

\end_layout

\begin_layout Standard

\backslash
altaffiltext{5}{Patron, Alonso's Bar and Grill}
\end_layout

\end_inset


\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 Standard

\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 Standard

\backslash
citep{kin75,new78}
\end_layout

\end_inset

 seemed a unique anomaly.
 Then 
\begin_inset ERT
status collapsed

\begin_layout Standard

\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 Standard

\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 Standard

\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 Standard

\backslash
citep{kin68,pet76,har84,ort85}
\end_layout

\end_inset

, as well as photoelectric profiles 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
citep{kin66,kin75}
\end_layout

\end_inset

 and electronographic profiles 
\begin_inset ERT
status collapsed

\begin_layout Standard

\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 Standard

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 LatexCommand \cite{hag86}

\end_inset

; we briefly summarize below.
\end_layout

\begin_layout Subsection

Formalism
\end_layout

\begin_layout Standard


\begin_inset LatexCommand \label{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 \( (\sigma =\pm 1) \)
\end_inset

, 
\begin_inset Formula \( \hat{a}_{i}=a^{\mu }_{i}\gamma _{\nu } \)
\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 \( a^{\mu }_{i} \)
\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 \( 2\times 2 \)
\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) ,\nonumber \\
\sigma ^{\mu }_{\pm } & = & ({\textbf {1}},\pm \sigma ),\nonumber
\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 ^{\mu }_{\pm },
\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\InsetSpace ~

\begin_inset LatexCommand \ref{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
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
degr
\backslash
 
\end_layout

\end_inset

out of phase with previous values.
 We have no observations of 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
ion{Ca}{2}
\end_layout

\end_inset

.
 Roughly 
\begin_inset ERT
status collapsed

\begin_layout Standard

\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\InsetSpace ~

\begin_inset LatexCommand \ref{bozomath}

\end_inset

.
 More information on the AASTeX macros package are available at 

\begin_inset LatexCommand \url{http://www.aas.org/publications/aastex}

\end_inset


 or the 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
\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
\bibitem [Auri\`ere(1982)]{aur82}

Auri\i \`{e}
re, M.
 1982, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
aap
\end_layout

\end_inset

, 109, 301 
\end_layout

\begin_layout References
\bibitem [Canizares et al.(1978)]{can78}

Canizares, C.
 R., Grindlay, J.
 E., Hiltner, W.
 A., Liller, W., and McClintock, J.
 E.
 1978, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
apj
\end_layout

\end_inset

, 224, 39 
\end_layout

\begin_layout References
\bibitem [Djorgovski and King(1984)]{djo84}

Djorgovski, S., and King, I.
 R.
 1984, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
apjl
\end_layout

\end_inset

, 277, L49 
\end_layout

\begin_layout References
\bibitem [Hagiwara and Zeppenfeld(1986)]{hag86}

Hagiwara, K., and Zeppenfeld, D.
 1986, Nucl.Phys., 274, 1 
\end_layout

\begin_layout References
\bibitem [Harris and van den Bergh(1984)]{har84}

Harris, W.
 E., and van den Bergh, S.
 1984, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
aj
\end_layout

\end_inset

, 89, 1816 
\end_layout

\begin_layout References
\bibitem [H\`enon(1961)]{hen61}

H\i \'{e}
non, M.
 1961, Ann.d'Ap., 24, 369 
\end_layout

\begin_layout References
\bibitem [King(1966)]{kin66}

King, I.
 R.
 1966, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
aj
\end_layout

\end_inset

, 71, 276 
\end_layout

\begin_layout References
\bibitem [King(1975)]{kin75}

King, I.
 R.
 1975, Dynamics of Stellar Systems, A.
 Hayli, Dordrecht: Reidel, 1975, 99 
\end_layout

\begin_layout References
\bibitem [King et al.(1968)]{kin68}

King, I.
 R., Hedemann, E., Hodge, S.
 M., and White, R.
 E.
 1968, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
aj
\end_layout

\end_inset

, 73, 456 
\end_layout

\begin_layout References
\bibitem [Kron et al.(1984)]{kro84}

Kron, G.
 E., Hewitt, A.
 V., and Wasserman, L.
 H.
 1984, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
pasp
\end_layout

\end_inset

, 96, 198 
\end_layout

\begin_layout References
\bibitem [Lynden-Bell and Wood(1968)]{lyn68}

Lynden-Bell, D., and Wood, R.
 1968, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
mnras
\end_layout

\end_inset

, 138, 495 
\end_layout

\begin_layout References
\bibitem [Newell and O'Neil(1978)]{new78}

Newell, E.
 B., and O'Neil, E.
 J.
 1978, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
apjs
\end_layout

\end_inset

, 37, 27 
\end_layout

\begin_layout References
\bibitem [Ortolani et al.(1985)]{ort85}

Ortolani, S., Rosino, L., and Sandage, A.
 1985, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
aj
\end_layout

\end_inset

, 90, 473 
\end_layout

\begin_layout References
\bibitem [Peterson(1976)]{pet76}

Peterson, C.
 J.
 1976, 
\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
aj
\end_layout

\end_inset

, 81, 617 
\end_layout

\begin_layout References
\bibitem [Spitzer(1985)]{spi85}

Spitzer, L.
 1985, Dynamics of Star Clusters, J.
 Goodman and P.
 Hut, Dordrecht: Reidel, 109 
\end_layout

\begin_layout Standard


\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
clearpage
\end_layout

\end_inset


\end_layout

\begin_layout FigCaption


\begin_inset LatexCommand \label{fig1}

\end_inset

This is the first figure and it uses sgi9259.eps as its EPS figure file.
\end_layout

\begin_layout FigCaption


\begin_inset LatexCommand \label{fig2}

\end_inset

This is an example of a long figure caption that must be set as a paragraph.
  The processor has to buffer the text of the caption, so it is good not
 to be too wordy, but that would make for poor communication as well.
 
\end_layout

\begin_layout FigCaption


\begin_inset LatexCommand \label{fig3}

\end_inset

This figure has no associated EPS file, so the optional parameter is omitted.
 
\end_layout

\begin_layout Standard


\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
clearpage
\end_layout

\end_inset


\end_layout

\begin_layout Standard

\begin_inset Float table
wide false
sideways false
status open

\begin_layout Caption

Terribly relevant tabular information.
\begin_inset LatexCommand \label{tbl-2}

\end_inset


\end_layout

\begin_layout Standard


\begin_inset VSpace medskip
\end_inset


\end_layout


\begin_layout Standard


\begin_inset  Tabular
<lyxtabular version="3" rows="7" columns="13">
<features endhead="-1" endfirsthead="-1" endfoot="-1" endlastfoot="-1">
<column alignment="center" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="right" valignment="top" width="0pt">
<column alignment="center" valignment="top" width="0pt">
<row>
<cell alignment="center" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

Star 
\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 Height 
\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( d_{x} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( d_{y} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( n \)
\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( \chi ^{2} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( R_{maj} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( R_{min} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell multicolumn="1" alignment="center" valignment="top" usebox="none">
\begin_inset Text

\begin_layout Standard


\begin_inset Formula \( P \)
\end_inset


\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
tablenotemark{a}
\end_layout

\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( PR_{maj} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text

\begin_layout Standard

 
\begin_inset Formula \( PR_{min} \)
\end_inset


\end_layout

\end_inset
</cell>
<cell multicolumn="1" alignment="center" valignment="top" usebox="none">
\begin_inset Text

\begin_layout Standard


\begin_inset Formula \( \Theta  \)
\end_inset


\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
tablenotemark{b}
\end_layout

\end_inset


\end_layout

\end_inset
</cell>
<cell alignment="center" valignment="top" usebox="none">
\begin_inset Text

\begin_layout Standard

Ref.
\end_layout

\end_inset
</cell>
</row>
<row>
<cell alignment="center" valignment="top" usebox="none">
\begin_inset Text

\begin_layout Standard


\begin_inset ERT
status collapsed

\begin_layout Standard

\backslash
tableline
\backslash
tableline
\end_layout

\end_inset

1 
\end_layout

\end_inset
</cell>
<cell alignment="right" valignment="top" usebox="none">
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33472.5 
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0.4 
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53 
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27.4 
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2.065 
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1.940 
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3.900 
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68.3 
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116.2 
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60 
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3.7 
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1.628 
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1.510 
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2.156 
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7.5 
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1.622 
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1.551 
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2.159 
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1.574 
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2.343 
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\backslash
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 table environment} 
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\end_layout

\begin_layout TableComments

We can also attach a long-ish paragraph of explanatory material to a table.
 Use 
\backslash
tablerefs to append a list of references.
 The following references were from a different table: I've patched them
 in here to show how they look, but don't take them too seriously---I certainly
 have not.
\end_layout

\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

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% LyX can load deluxetable files verbatim.
 To see this in action, uncomment the following
\end_layout

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% line (delete the 
\end_layout

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\begin_inset Quotes eld
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%
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\begin_inset Quotes erd
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) and copy the file table.tex from the AASTeX 5.0 distribution into
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% the same directory as this file.
\end_layout

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%
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\begin_inset Include \input{table}

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\end_body
\end_document