-#LyX 1.3 created this file. For more info see http://www.lyx.org/
-\lyxformat 221
+#LyX 1.5.0svn created this file. For more info see http://www.lyx.org/
+\lyxformat 245
+\begin_document
+\begin_header
\textclass aastex
\begin_preamble
\newcommand{\vdag}{(v)^\dagger}
\graphics default
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\spacing single
-\papersize Default
-\paperpackage a4
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+\use_bibtopic false
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\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
-\layout Title
+\begin_body
+
+\begin_layout Title
Collapsed Cores in Globular Clusters, Gauge-Boson Couplings, and AASTeX
Examples
-\layout Author
+\end_layout
+
+\begin_layout Author
S.
Djorgovski
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
altaffilmark{1,2,3}
-\end_inset
+\end_layout
+
+\end_inset
and Ivan R.
King
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
altaffilmark{1}
-\end_inset
+\end_layout
+
+\end_inset
-\layout Affiliation
+\end_layout
+
+\begin_layout Affiliation
Astronomy Department, University of California, Berkeley, CA 94720
-\layout Author
+\end_layout
+
+\begin_layout Author
C.
D.
Biemesderfer
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
altaffilmark{4,5}
-\end_inset
+\end_layout
+
+\end_inset
+
+\end_layout
-\layout Affiliation
+\begin_layout Affiliation
National Optical Astronomy Observatories, Tucson, AZ 85719
-\layout Email
+\end_layout
+
+\begin_layout Email
aastex-help@aas.org
-\layout And
+\end_layout
+
+\begin_layout And
-\layout Author
+\end_layout
+
+\begin_layout Author
R.
J.
Hanisch
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
altaffilmark{5}
-\end_inset
+\end_layout
+
+\end_inset
-\layout Affiliation
+\end_layout
+
+\begin_layout Affiliation
Space Telescope Science Institute, Baltimore, MD 21218
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
altaffiltext{1}{Visiting Astronomer, Cerro Tololo Inter-American Observatory.
CTIO is operated by AURA, Inc.
-\backslash
+\backslash
under contract to the National Science Foundation.}
-\layout Standard
+\end_layout
+
+\begin_layout Standard
-\backslash
+\end_layout
+
+\begin_layout Standard
+
+\backslash
altaffiltext{2}{Society of Fellows, Harvard University.}
-\layout Standard
+\end_layout
+
+\begin_layout Standard
+
+\end_layout
-\backslash
+\begin_layout Standard
+
+\backslash
altaffiltext{3}{present address: Center for Astrophysics, 60 Garden Street,
Cambridge, MA 02138}
-\layout Standard
+\end_layout
+
+\begin_layout Standard
+
+\end_layout
-\backslash
+\begin_layout Standard
+
+\backslash
altaffiltext{4}{Visiting Programmer, Space Telescope Science Institute}
-\layout Standard
+\end_layout
+
+\begin_layout Standard
+
+\end_layout
+
+\begin_layout Standard
-\backslash
+\backslash
altaffiltext{5}{Patron, Alonso's Bar and Grill}
-\end_inset
+\end_layout
+\end_inset
-\layout Abstract
+
+\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.
-\layout Keywords
+\end_layout
+
+\begin_layout Keywords
clusters: globular, peanut---bosons: bozos
-\layout Section
+\end_layout
+
+\begin_layout Section
Introduction
-\layout Standard
+\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
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep{hen61,lyn68,spi85}
-\end_inset
+\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
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep{kin75,new78}
-\end_inset
+\end_layout
+
+\end_inset
seemed a unique anomaly.
Then
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citet{aur82}
-\end_inset
+\end_layout
+
+\end_inset
suggested a central peak in NGC 6397, and a limited photographic survey
of ours
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep[Paper I]{djo84}
-\end_inset
+\end_layout
+
+\end_inset
found three more cases, including NGC 6624, whose sharp center had often
been remarked on
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep{can78}
-\end_inset
+\end_layout
+
+\end_inset
.
-\layout Section
+\end_layout
+
+\begin_layout Section
Observations
-\layout Standard
+\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
+\end_inset
500 chip and a GEC 575
\begin_inset Formula \( \times \)
-\end_inset
+\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
+\end_inset
385, with
\begin_inset Formula \( B,V, \)
-\end_inset
+\end_inset
and
\begin_inset Formula \( R \)
-\end_inset
+\end_inset
filters, and an RCA 512
\begin_inset Formula \( \times \)
-\end_inset
+\end_inset
320, with
\begin_inset Formula \( U,B,V,R, \)
-\end_inset
+\end_inset
and
\begin_inset Formula \( I \)
-\end_inset
+\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
+\end_inset
or even in
\begin_inset Formula \( B \)
-\end_inset
+\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
+\end_layout
+
+\begin_layout Standard
The CCD images are unfortunately not always suitable, for very poor clusters
or for clusters with large cores.
CCD profiles by collecting from the literature a number of star-count profiles
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep{kin68,pet76,har84,ort85}
-\end_inset
+\end_layout
+
+\end_inset
, as well as photoelectric profiles
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep{kin66,kin75}
-\end_inset
+\end_layout
+
+\end_inset
and electronographic profiles
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
citep{kro84}
-\end_inset
+\end_layout
+
+\end_inset
.
In a few cases we judged normality by eye estimates on one of the Sky Surveys.
-\layout Section
+\end_layout
+
+\begin_layout Section
Helicity Amplitudes
-\layout Standard
+\end_layout
+
+\begin_layout Standard
It has been realized that helicity amplitudes provide a convenient means
for Feynman diagram
\begin_inset Foot
-collapsed true
+status collapsed
-\layout Standard
+\begin_layout Standard
Footnotes can be inserted like this.
-\end_inset
+\end_layout
+
+\end_inset
evaluations.
These amplitude-level techniques are particularly convenient for calculations
\begin_inset LatexCommand \cite{hag86}
-\end_inset
+\end_inset
; we briefly summarize below.
-\layout Subsection
+\end_layout
+
+\begin_layout Subsection
Formalism
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset LatexCommand \label{bozomath}
-\end_inset
+\end_inset
-\layout Standard
+\end_layout
+
+\begin_layout Standard
A tree-level amplitude in
\begin_inset Formula \( e^{+}e^{-} \)
-\end_inset
+\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
+\end_inset
where
\begin_inset Formula \( p \)
-\end_inset
+\end_inset
and
\begin_inset Formula \( \sigma \)
-\end_inset
+\end_inset
label the initial
\begin_inset Formula \( e^{\pm } \)
-\end_inset
+\end_inset
four-momenta and helicities
\begin_inset Formula \( (\sigma =\pm 1) \)
-\end_inset
+\end_inset
,
\begin_inset Formula \( \hat{a}_{i}=a^{\mu }_{i}\gamma _{\nu } \)
-\end_inset
+\end_inset
and
\begin_inset Formula \( P_{\tau }=\frac{1}{2}(1+\tau \gamma _{5}) \)
-\end_inset
+\end_inset
is a chirality projection operator
\begin_inset Formula \( (\tau =\pm1 ) \)
-\end_inset
+\end_inset
.
The
\begin_inset Formula \( a^{\mu }_{i} \)
-\end_inset
+\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
+\end_layout
+
+\begin_layout NoteToEditor
Figures 1 and 2 should appear side-by-side in print
-\layout Standard
+\end_layout
+
+\begin_layout Standard
In the chiral representation the
\begin_inset Formula \( \gamma \)
-\end_inset
+\end_inset
matrices are expressed in terms of
\begin_inset Formula \( 2\times 2 \)
-\end_inset
+\end_inset
Pauli matrices
\begin_inset Formula \( \sigma \)
-\end_inset
+\end_inset
and the unit matrix 1 as
\begin_inset Formula \begin{eqnarray}
-1 & 0\\
0 & 1
\end{array}\right) ,\nonumber \\
-\sigma ^{\mu }_{\pm } & = & ({\textbf {1}},\pm \sigma ),\nonumber
+\sigma ^{\mu }_{\pm } & = & ({\textbf {1}},\pm \sigma ),\nonumber
\end{eqnarray}
-\end_inset
+\end_inset
giving
\begin_inset Formula \begin{equation}
\end{array}\right) ,(\hat{a})_{\pm }=a_{\mu }\sigma ^{\mu }_{\pm },
\end{equation}
-\end_inset
+\end_inset
The spinors are expressed in terms of two-component Weyl spinors as
\begin_inset Formula \begin{equation}
\end{array}\right) ,v={\textbf {(}}\vdag _{+}{\textbf {,}}\vdag _{-}{\textbf {)}}.
\end{equation}
-\end_inset
+\end_inset
-\layout Standard
+\end_layout
+
+\begin_layout Standard
The Weyl spinors are given in terms of helicity eigenstates
\begin_inset Formula \( \chi _{\lambda }(p) \)
-\end_inset
+\end_inset
with
\begin_inset Formula \( \lambda =\pm1 \)
-\end_inset
+\end_inset
by
-\layout MathLetters
+\end_layout
+
+\begin_layout MathLetters
\begin_inset Formula \begin{eqnarray}
v(p,\lambda )_{\pm } & = & \pm \lambda (E\mp \lambda |{\textbf {p}}|)^{1/2}\chi _{-\lambda }(p)
\end{eqnarray}
-\end_inset
+\end_inset
-\layout Section
+\end_layout
+
+\begin_layout Section
Floating material and so forth
-\layout Standard
+\end_layout
+
+\begin_layout Standard
Consider a task that computes profile parameters for a modified Lorentzian
of the form
I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
\end{equation}
-\end_inset
+\end_inset
where
\begin_inset Formula \[
\frac{y_{1}}{R_{min}}
\end{array}\right) ^{2}}\]
-\end_inset
+\end_inset
\begin_inset Formula \[
\case {y_{1}}{PR_{min}}
\end{array}\right) ^{2}}\]
-\end_inset
+\end_inset
\begin_inset Formula \[
x_{1}=(x-x_{0})\cos \Theta +(y-y_{0})\sin \Theta \]
-\end_inset
+\end_inset
\begin_inset Formula \[
y_{1}=-(x-x_{0})\sin \Theta +(y-y_{0})\cos \Theta \]
-\end_inset
+\end_inset
-\layout Standard
+\end_layout
+
+\begin_layout Standard
In these expressions
\begin_inset Formula \( x_{0} \)
-\end_inset
+\end_inset
,
\begin_inset Formula \( y_{0} \)
-\end_inset
+\end_inset
is the star center, and
\begin_inset Formula \( \Theta \)
-\end_inset
+\end_inset
is the angle with the
\begin_inset Formula \( x \)
-\end_inset
+\end_inset
axis.
- Results of this task are shown in table\SpecialChar ~
+ Results of this task are shown in table\InsetSpace ~
\begin_inset LatexCommand \ref{tbl-2}
-\end_inset
+\end_inset
.
It is not clear how these sorts of analyses may affect determination of
\begin_inset Formula \( M_{\sun } \)
-\end_inset
+\end_inset
, but the assumption is that the alternate results should be less than 90
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
degr
-\backslash
+\backslash
-\end_inset
+\end_layout
+
+\end_inset
out of phase with previous values.
We have no observations of
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
ion{Ca}{2}
-\end_inset
+\end_layout
+
+\end_inset
.
Roughly
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
slantfrac{4}{5}
-\end_inset
+\end_layout
+
+\end_inset
of the electronically submitted abstracts for AAS meetings are error-free.
-\layout Acknowledgements
+\end_layout
+
+\begin_layout Acknowledgements
-\layout Standard
+\end_layout
+
+\begin_layout Standard
We are grateful to V.
Barger, T.
Han, and R.
J.
N.
- Phillips for doing the math in section\SpecialChar ~
+ Phillips for doing the math in section\InsetSpace ~
\begin_inset LatexCommand \ref{bozomath}
-\end_inset
+\end_inset
.
More information on the AASTeX macros package are available at
\begin_inset LatexCommand \url{http://www.aas.org/publications/aastex}
-\end_inset
+\end_inset
or the
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
anchor{ftp://www.aas.org/pubs/}{AAS ftp site}
-\end_inset
+\end_layout
+
+\end_inset
.
-\layout Appendix
+\end_layout
-\layout Section
+\begin_layout Appendix
+
+\end_layout
+
+\begin_layout Section
Appendicial material
-\layout Standard
+\end_layout
+
+\begin_layout Standard
Consider once again a task that computes profile parameters for a modified
Lorentzian of the form
I=\frac{1}{1+d_{1}^{P(1+d_{2})}}
\end{equation}
-\end_inset
+\end_inset
where
-\layout MathLetters
+\end_layout
+
+\begin_layout MathLetters
\begin_inset Formula \[
\frac{y_{1}}{R_{min}}
\end{array}\right) ^{2}}\]
-\end_inset
+\end_inset
\begin_inset Formula \begin{equation}
\end{array}\right) ^{2}}
\end{equation}
-\end_inset
+\end_inset
\begin_inset Formula \begin{eqnarray}
y_{1} & = & -(x-x_{0})\sin \Theta +(y-y_{0})\cos \Theta
\end{eqnarray}
-\end_inset
+\end_inset
+
+\end_layout
-\layout Standard
+\begin_layout Standard
For completeness, here is one last equation.
e=mc^{2}
\end{equation}
-\end_inset
+\end_inset
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Auri\`ere(1982)]{aur82}
Auri\i \`{e}
re, M.
1982,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
aap
-\end_inset
+\end_layout
+
+\end_inset
, 109, 301
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Canizares et al.(1978)]{can78}
Canizares, C.
E.
1978,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
apj
-\end_inset
+\end_layout
+
+\end_inset
, 224, 39
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Djorgovski and King(1984)]{djo84}
Djorgovski, S., and King, I.
R.
1984,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
apjl
-\end_inset
+\end_layout
+
+\end_inset
, 277, L49
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Hagiwara and Zeppenfeld(1986)]{hag86}
Hagiwara, K., and Zeppenfeld, D.
1986, Nucl.Phys., 274, 1
-\layout References
+\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
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
aj
-\end_inset
+\end_layout
+
+\end_inset
, 89, 1816
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [H\`enon(1961)]{hen61}
H\i \'{e}
non, M.
1961, Ann.d'Ap., 24, 369
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [King(1966)]{kin66}
King, I.
R.
1966,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
aj
-\end_inset
+\end_layout
+
+\end_inset
, 71, 276
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [King(1975)]{kin75}
King, I.
R.
1975, Dynamics of Stellar Systems, A.
Hayli, Dordrecht: Reidel, 1975, 99
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [King et al.(1968)]{kin68}
King, I.
E.
1968,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
aj
-\end_inset
+\end_layout
+
+\end_inset
, 73, 456
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Kron et al.(1984)]{kro84}
Kron, G.
H.
1984,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
pasp
-\end_inset
+\end_layout
+
+\end_inset
, 96, 198
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Lynden-Bell and Wood(1968)]{lyn68}
Lynden-Bell, D., and Wood, R.
1968,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
mnras
-\end_inset
+\end_layout
+
+\end_inset
, 138, 495
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Newell and O'Neil(1978)]{new78}
Newell, E.
J.
1978,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
apjs
-\end_inset
+\end_layout
+
+\end_inset
, 37, 27
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Ortolani et al.(1985)]{ort85}
Ortolani, S., Rosino, L., and Sandage, A.
1985,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
aj
-\end_inset
+\end_layout
+
+\end_inset
, 90, 473
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Peterson(1976)]{pet76}
Peterson, C.
J.
1976,
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
aj
-\end_inset
+\end_layout
+
+\end_inset
, 81, 617
-\layout References
+\end_layout
+
+\begin_layout References
\bibitem [Spitzer(1985)]{spi85}
Spitzer, L.
1985, Dynamics of Star Clusters, J.
Goodman and P.
Hut, Dordrecht: Reidel, 109
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
clearpage
-\end_inset
+\end_layout
+
+\end_inset
-\layout FigCaption
+\end_layout
+
+\begin_layout FigCaption
\begin_inset LatexCommand \label{fig1}
-\end_inset
+\end_inset
This is the first figure and it uses sgi9259.eps as its EPS figure file.
-\layout FigCaption
+\end_layout
+
+\begin_layout FigCaption
\begin_inset LatexCommand \label{fig2}
-\end_inset
+\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
+\end_layout
+
+\begin_layout FigCaption
\begin_inset LatexCommand \label{fig3}
-\end_inset
+\end_inset
This figure has no associated EPS file, so the optional parameter is omitted.
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
-\backslash
+\backslash
clearpage
-\end_inset
+\end_layout
+
+\end_inset
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset Float table
wide false
-collapsed false
+sideways false
+status open
+
+\begin_layout Caption
-\layout Caption
-\added_space_bottom medskip
Terribly relevant tabular information.
\begin_inset LatexCommand \label{tbl-2}
-\end_inset
+\end_inset
+
+
+\end_layout
+
+\begin_layout Standard
+
+
+\begin_inset VSpace medskip
+\end_inset
-\layout Standard
+\end_layout
+
+
+\begin_layout Standard
\begin_inset Tabular
<cell alignment="center" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
-\layout Standard
+\begin_layout Standard
Star
-\end_inset
+\end_layout
+
+\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
-\layout Standard
+\begin_layout Standard
Height
-\end_inset
+\end_layout
+
+\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
-\layout Standard
+\begin_layout Standard
\begin_inset Formula \( d_{x} \)
-\end_inset
+\end_inset
-\end_inset
+\end_layout
+
+\end_inset
</cell>
<cell alignment="right" valignment="top" topline="true" bottomline="true" usebox="none">
\begin_inset Text
-\layout Standard
+\begin_layout Standard
\begin_inset Formula \( d_{y} \)
-\end_inset
+\end_inset
+
+\end_layout
-\end_inset
+\end_inset
</cell>
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+
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</cell>
<cell multicolumn="1" alignment="center" valignment="top" usebox="none">
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</cell>
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Ref.
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1
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33472.5
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27.4
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2.065
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1.940
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</cell>
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3.900
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+
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</cell>
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68.3
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116.2
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27802.4
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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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6.8
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7.5
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29210.6
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3.4
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1.622
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1.551
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2.159
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32733.8
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54.8
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2.282
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4.313
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117.4
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78.2
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-35.847
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5
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9607.4
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60
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1.4
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1.669
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1.574
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2.343
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8.0
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8.9
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7
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6
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31638.6
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1.6
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39
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+
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<cell alignment="right" valignment="top" bottomline="true" usebox="none">
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315.2
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+
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3.433
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+
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3.075
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+
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7.488
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+
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+
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25.3
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<cell alignment="right" valignment="top" bottomline="true" usebox="none">
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8
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+
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</row>
</lyxtabular>
-\end_inset
+\end_inset
+
+\end_layout
-\layout Standard
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
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-\layout Standard
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-\backslash
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tablenotetext{a}{Sample footnote for table~
-\backslash
+\backslash
ref{tbl-2} that was generated with the
-\backslash
+\backslash
LaTeX
-\backslash
+\backslash
table environment}
-\layout Standard
+\end_layout
-\backslash
+\begin_layout Standard
+
+\end_layout
+
+\begin_layout Standard
+
+\backslash
tablenotetext{b}{Yet another sample footnote for table~
-\backslash
+\backslash
ref{tbl-2}}
-\layout Standard
+\end_layout
+
+\begin_layout Standard
-\backslash
+\end_layout
+
+\begin_layout Standard
+
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tablenotetext{c}{Another sample footnote for table~
-\backslash
+\backslash
ref{tbl-2}}
-\end_inset
+\end_layout
+
+\end_inset
-\layout TableComments
+\end_layout
+
+\begin_layout TableComments
We can also attach a long-ish paragraph of explanatory material to a table.
Use
-\backslash
+\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
+\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.
1984; (23) Spite & Spite 1986; (24) Hobbs & Thorburn 1991; (25) Hobbs et
al.
1991; (26) Olsen 1983.
-\end_inset
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+
+\end_inset
+
+\end_layout
-\layout Standard
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
% LyX can load deluxetable files verbatim.
To see this in action, uncomment the following
-\end_inset
+\end_layout
+\end_inset
-\layout Standard
+
+\end_layout
+
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
% line (delete the
-\end_inset
+\end_layout
+
+\end_inset
\begin_inset Quotes eld
-\end_inset
+\end_inset
\begin_inset ERT
-status Collapsed
+status collapsed
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+\begin_layout Standard
%
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+
+\end_inset
\begin_inset Quotes erd
-\end_inset
+\end_inset
\begin_inset ERT
-status Collapsed
+status collapsed
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+\begin_layout Standard
) and copy the file table.tex from the AASTeX 5.0 distribution into
-\end_inset
+\end_layout
+
+\end_inset
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
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+\begin_layout Standard
% the same directory as this file.
-\end_inset
+\end_layout
+
+\end_inset
-\layout Standard
+\end_layout
+
+\begin_layout Standard
\begin_inset ERT
-status Collapsed
+status collapsed
-\layout Standard
+\begin_layout Standard
%
-\end_inset
+\end_layout
+
+\end_inset
\begin_inset Include \input{table}
-\end_inset
+\end_inset
+
+\end_layout
-\the_end
+\end_body
+\end_document
projects / lyx.git / blobdiff