#This file was created by 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 english \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 0 0 0 0 8 0 0 "" "" 4 0 0 "" "" 4 0 0 "" "" 4 0 0 "" "" 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 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 1 8 0 0 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 0 4 1 1 0 0 0 "" "" 1 8 0 0 0 0 0 "" "" 0 8 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 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 \layout Standard \latex latex % LyX can load deluxetable files verbatim. To see this in action, uncomment the following \layout Standard \latex latex % line (delete the \latex default \begin_inset Quotes eld \end_inset \latex latex % \latex default \begin_inset Quotes erd \end_inset \latex latex ) and copy the file table.tex from the AASTeX 5.0 distribution into \layout Standard \latex latex % the same directory as this file. \layout Standard \latex latex % \begin_inset Include \input{table} \end_inset \the_end