#This file was created by <mike> Sun Jul 25 23:59:27 1999
#LyX 1.0 (C) 1995-1999 Matthias Ettrich and the LyX Team
\lyxformat 2.15
\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 default
\inputencoding default
\fontscheme default
\graphics default
\paperfontsize default
\spacing single 
\papersize Default
\paperpackage a4
\use_geometry 0
\use_amsmath 0
\paperorientation portrait
\secnumdepth 3
\tocdepth 3
\paragraph_separation indent
\defskip medskip
\quotes_language english
\quotes_times 2
\papercolumns 1
\papersides 1
\paperpagestyle default

\layout Title

Collapsed Cores in Globular Clusters,  Gauge-Boson Couplings, and AASTeX
\latex latex 
 
\latex default 
Examples
\layout Author

S.
 Djorgovski
\latex latex 

\backslash 
altaffilmark{1,2,3}
\latex default 
 and Ivan R.
 King
\latex latex 

\backslash 
altaffilmark{1}
\layout Affiliation

Astronomy Department, University of California, Berkeley, CA 94720
\layout Author

C.
 D.
 Biemesderfer
\latex latex 

\backslash 
altaffilmark{4,5}
\layout Affiliation

National Optical Astronomy Observatories, Tucson, AZ 85719
\layout Email

aastex-help@aas.org
\layout And

\layout Author

R.
 J.
 Hanisch
\latex latex 

\backslash 
altaffilmark{5}
\layout Affiliation

Space Telescope Science Institute, Baltimore, MD 21218
\layout Standard


\latex latex 

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


\latex latex 

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


\latex latex 

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


\latex latex 

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


\latex latex 

\backslash 
altaffiltext{5}{Patron, Alonso's Bar and Grill}
\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.
 
\layout Keywords

clusters: globular, peanut---bosons: bozos
\layout Section

Introduction
\layout Standard

A focal problem today in the dynamics of globular clusters is core collapse.
 It has been predicted by theory for decades 
\latex latex 

\backslash 
citep{hen61,lyn68,spi85}
\latex default 
, but observation has been less alert to the phenomenon.
 For many years the central brightness peak in M15 
\latex latex 

\backslash 
citep{kin75,new78}
\latex default 
 seemed a unique anomaly.
 Then 
\latex latex 

\backslash 
citet{aur82}
\latex default 
 suggested a central peak in NGC 6397, and a limited photographic survey
 of ours 
\latex latex 

\backslash 
citep[Paper I]{djo84}
\latex default 
 found three more cases, including NGC 6624, whose sharp center had often
 been remarked on 
\latex latex 

\backslash 
citep{can78}
\latex default 
.
 
\layout Section

Observations
\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.
\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
 
\latex latex 

\backslash 
citep{kin68,pet76,har84,ort85}
\latex default 
, as well as photoelectric profiles 
\latex latex 

\backslash 
citep{kin66,kin75}
\latex default 
 and electronographic profiles 
\latex latex 

\backslash 
citep{kro84}
\latex default 
.
 In a few cases we judged normality by eye estimates on one of the Sky Surveys.
\layout Section

Helicity Amplitudes
\layout Standard

It has been realized that helicity amplitudes provide a convenient means
 for Feynman diagram
\begin_float footnote 
\layout Standard

Footnotes can be inserted like this.
\end_float 
 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.
\layout Subsection

Formalism
\layout Standard


\begin_inset LatexCommand \label{bozomath}

\end_inset 


\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.
\layout NoteToEditor

Figures 1 and 2 should appear side-by-side in print
\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 


\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 
\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 


\layout Section

Floating material and so forth
\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 


\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
\protected_separator 

\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
\latex latex 

\backslash 
degr
\backslash 
 
\latex default 
out of phase with previous values.
 We have no observations of 
\latex latex 

\backslash 
ion{Ca}{2}
\latex default 
.
 Roughly 
\latex latex 

\backslash 
slantfrac{4}{5}
\latex default 
 of the electronically submitted abstracts for AAS meetings are error-free.
\layout Acknowledgements

\layout Standard

We are grateful to V.
 Barger, T.
 Han, and R.
 J.
 N.
 Phillips for doing the math in section
\protected_separator 

\begin_inset LatexCommand \ref{bozomath}

\end_inset 

.
 More information on the AASTeX macros package are available at 
\latex latex 

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

\end_inset 


\latex default 
 or the 
\latex latex 

\backslash 
anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
\latex default 
.
\layout Appendix

\layout Section

Appendicial material
\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 
\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 


\layout Standard

For completeness, here is one last equation.
 
\begin_inset Formula 
\begin{equation}
e=mc^{2}
\end{equation}

\end_inset 


\layout References
\bibitem [Auri\`ere(1982)]{aur82}

Auri\i \`{e}
re, M.
 1982, 
\latex latex 

\backslash 
aap
\latex default 
, 109, 301 
\layout References
\bibitem [Canizares et al.(1978)]{can78}

Canizares, C.
 R., Grindlay, J.
 E., Hiltner, W.
 A., Liller, W., and McClintock, J.
 E.
 1978, 
\latex latex 

\backslash 
apj
\latex default 
, 224, 39 
\layout References
\bibitem [Djorgovski and King(1984)]{djo84}

Djorgovski, S., and King, I.
 R.
 1984, 
\latex latex 

\backslash 
apjl
\latex default 
, 277, L49 
\layout References
\bibitem [Hagiwara and Zeppenfeld(1986)]{hag86}

Hagiwara, K., and Zeppenfeld, D.
 1986, Nucl.Phys., 274, 1 
\layout References
\bibitem [Harris and van den Bergh(1984)]{har84}

Harris, W.
 E., and van den Bergh, S.
 1984, 
\latex latex 

\backslash 
aj
\latex default 
, 89, 1816 
\layout References
\bibitem [H\`enon(1961)]{hen61}

H\i \'{e}
non, M.
 1961, Ann.d'Ap., 24, 369 
\layout References
\bibitem [King(1966)]{kin66}

King, I.
 R.
 1966, 
\latex latex 

\backslash 
aj
\latex default 
, 71, 276 
\layout References
\bibitem [King(1975)]{kin75}

King, I.
 R.
 1975, Dynamics of Stellar Systems, A.
 Hayli, Dordrecht: Reidel, 1975, 99 
\layout References
\bibitem [King et al.(1968)]{kin68}

King, I.
 R., Hedemann, E., Hodge, S.
 M., and White, R.
 E.
 1968, 
\latex latex 

\backslash 
aj
\latex default 
, 73, 456 
\layout References
\bibitem [Kron et al.(1984)]{kro84}

Kron, G.
 E., Hewitt, A.
 V., and Wasserman, L.
 H.
 1984, 
\latex latex 

\backslash 
pasp
\latex default 
, 96, 198 
\layout References
\bibitem [Lynden-Bell and Wood(1968)]{lyn68}

Lynden-Bell, D., and Wood, R.
 1968, 
\latex latex 

\backslash 
mnras
\latex default 
, 138, 495 
\layout References
\bibitem [Newell and O'Neil(1978)]{new78}

Newell, E.
 B., and O'Neil, E.
 J.
 1978, 
\latex latex 

\backslash 
apjs
\latex default 
, 37, 27 
\layout References
\bibitem [Ortolani et al.(1985)]{ort85}

Ortolani, S., Rosino, L., and Sandage, A.
 1985, 
\latex latex 

\backslash 
aj
\latex default 
, 90, 473 
\layout References
\bibitem [Peterson(1976)]{pet76}

Peterson, C.
 J.
 1976, 
\latex latex 

\backslash 
aj
\latex default 
, 81, 617 
\layout References
\bibitem [Spitzer(1985)]{spi85}

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


\latex latex 

\backslash 
clearpage
\layout FigCaption


\begin_inset LatexCommand \label{fig1}

\end_inset 

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


\begin_inset LatexCommand \label{fig3}

\end_inset 

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


\latex latex 

\backslash 
clearpage
\layout Standard

\begin_float tab 
\layout Caption
\added_space_bottom medskip 
Terribly relevant tabular information.
\begin_inset LatexCommand \label{tbl-2}

\end_inset 


\layout Standard
\LyXTable
multicol5
7 13 0 0 -1 -1 -1 -1
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
0 0 0 0
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4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
4 0 0 "" ""
8 0 0 "" ""
0 8 1 1 0 0 0 "" ""
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1 8 0 0 0 0 0 "" ""
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1 8 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
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0 4 0 0 0 0 0 "" ""
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0 4 0 0 0 0 0 "" ""
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0 4 0 0 0 0 0 "" ""
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0 4 0 0 0 0 0 "" ""
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0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 4 0 0 0 0 0 "" ""
0 8 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""
0 4 0 1 0 0 0 "" ""

Star 
\newline 
 Height 
\newline 
 
\begin_inset Formula \( d_{x} \)
\end_inset 


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


\newline 
 
\begin_inset Formula \( n \)
\end_inset 


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


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


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


\newline 

\begin_inset Formula \( P \)
\end_inset 


\latex latex 

\backslash 
tablenotemark{a}
\latex default 

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


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


\newline 

\begin_inset Formula \( \Theta  \)
\end_inset 


\latex latex 

\backslash 
tablenotemark{b}
\latex default 

\newline 
Ref.
\newline 

\latex latex 

\backslash 
tableline
\backslash 
tableline
\latex default 
1 
\newline 
33472.5 
\newline 
-0.1 
\newline 
0.4 
\newline 
53 
\newline 
27.4 
\newline 
2.065 
\newline 
1.940 
\newline 
3.900 
\newline 
68.3 
\newline 
116.2 
\newline 
-27.639
\newline 
1,2
\newline 
 2 
\newline 
27802.4 
\newline 
-0.3 
\newline 
-0.2 
\newline 
60 
\newline 
3.7 
\newline 
1.628 
\newline 
1.510 
\newline 
2.156 
\newline 
6.8 
\newline 
7.5 
\newline 
-26.764
\newline 
3
\newline 
 3 
\newline 
29210.6 
\newline 
0.9 
\newline 
0.3 
\newline 
60 
\newline 
3.4 
\newline 
1.622 
\newline 
1.551 
\newline 
2.159 
\newline 
6.7 
\newline 
7.3 
\newline 
-40.272
\newline 
4
\newline 
 4 
\newline 
32733.8 
\newline 
-1.2
\latex latex 

\backslash 
tablenotemark{c}
\latex default 

\newline 
-0.5 
\newline 
41 
\newline 
54.8 
\newline 
2.282 
\newline 
2.156 
\newline 
4.313 
\newline 
117.4 
\newline 
78.2 
\newline 
-35.847
\newline 
5,6
\newline 
 5 
\newline 
 9607.4 
\newline 
-0.4 
\newline 
-0.4 
\newline 
60 
\newline 
1.4 
\newline 
1.669
\latex latex 

\backslash 
tablenotemark{c}
\latex default 

\newline 
1.574 
\newline 
2.343 
\newline 
8.0 
\newline 
8.9 
\newline 
-33.417
\newline 
7
\newline 
 6 
\newline 
31638.6 
\newline 
1.6 
\newline 
0.1 
\newline 
39 
\newline 
315.2 
\newline 
 3.433 
\newline 
3.075 
\newline 
7.488 
\newline 
92.1 
\newline 
25.3 
\newline 
-12.052 
\newline 
8
\layout Standard


\latex latex 

\backslash 
tablenotetext{a}{Sample footnote for table~
\backslash 
ref{tbl-2} that was generated with the 
\backslash 
LaTeX
\backslash 
 table environment} 
\layout Standard


\latex latex 

\backslash 
tablenotetext{b}{Yet another sample footnote for table~
\backslash 
ref{tbl-2}} 
\layout Standard


\latex latex 

\backslash 
tablenotetext{c}{Another sample footnote for table~
\backslash 
ref{tbl-2}}
\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.
\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_float 
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