From: Juergen Spitzmueller Date: Tue, 5 Mar 2024 14:52:22 +0000 (+0100) Subject: Fix file name X-Git-Url: https://git.lyx.org/gitweb/?a=commitdiff_plain;h=503bc42d7e70b97a81fa9706c2b51c211e14bd0e;p=features.git Fix file name This way, we still have a string freeze break, but it is at least only one string :-( (and no, it does not matter whether the translation of this string is identical to the English string) --- diff --git a/lib/Makefile.am b/lib/Makefile.am index e687ab1fe7..4ad1745aa7 100644 --- a/lib/Makefile.am +++ b/lib/Makefile.am @@ -370,7 +370,7 @@ dist_examples_DATA = \ articleexamplesdir = $(pkgdatadir)/examples/Articles dist_articleexamples_DATA = \ examples/Articles/Astronomy_%26_Astrophysics.lyx \ - examples/Articles/American_Astronomical_Society_%28AASTeX_v._631%29.lyx \ + examples/Articles/American_Astronomical_Society_%28AASTeX_v._6.3.1%29.lyx \ examples/Articles/American_Chemical_Society_%28ACS%29.lyx \ examples/Articles/American_Mathematical_Society_%28AMS%29.lyx @@ -2765,7 +2765,7 @@ dist_templates_DATA = \ articletemplatesdir = $(pkgdatadir)/templates/Articles dist_articletemplates_DATA = \ - templates/Articles/American_Astronomical_Society_%28AASTeX_v._631%29.lyx \ + templates/Articles/American_Astronomical_Society_%28AASTeX_v._6.3.1%29.lyx \ templates/Articles/American_Economic_Association_%28AEA%29.lyx \ templates/Articles/American_Psychological_Association_%28APA%29.lyx \ templates/Articles/American_Psychological_Association_%28APA%29,_v._7.lyx \ diff --git a/lib/examples/Articles/American_Astronomical_Society_%28AASTeX_v._6.3.1%29.lyx b/lib/examples/Articles/American_Astronomical_Society_%28AASTeX_v._6.3.1%29.lyx new file mode 100644 index 0000000000..8480811464 --- /dev/null +++ b/lib/examples/Articles/American_Astronomical_Society_%28AASTeX_v._6.3.1%29.lyx @@ -0,0 +1,2565 @@ +#LyX 2.4 created this file. For more info see https://www.lyx.org/ +\lyxformat 620 +\begin_document +\begin_header +\save_transient_properties true +\origin unavailable +\textclass aastex63 +\begin_preamble +\newcommand{\myemail}{skywalker@galaxy.far.far.away} +%\slugcomment{Not to appear in Nonlearned J., 45.} +\shorttitle{Djorgovski et al.} +\shortauthors{Collapsed Cores in Globular Clusters} +\end_preamble +\use_default_options true +\maintain_unincluded_children no +\language english +\language_package default +\inputencoding utf8 +\fontencoding auto +\font_roman "default" "default" +\font_sans "default" "default" +\font_typewriter "default" "default" +\font_math "auto" "auto" +\font_default_family default +\use_non_tex_fonts false +\font_sc false +\font_roman_osf false +\font_sans_osf false +\font_typewriter_osf false +\font_sf_scale 100 100 +\font_tt_scale 100 100 +\use_microtype false +\use_dash_ligatures false +\graphics default +\default_output_format default +\output_sync 0 +\bibtex_command default +\index_command default +\float_placement class +\float_alignment class +\paperfontsize default +\spacing single +\use_hyperref false +\papersize default +\use_geometry false +\use_package amsmath 1 +\use_package amssymb 1 +\use_package cancel 1 +\use_package esint 1 +\use_package mathdots 1 +\use_package mathtools 1 +\use_package mhchem 1 +\use_package stackrel 1 +\use_package stmaryrd 1 +\use_package undertilde 1 +\cite_engine natbib +\cite_engine_type authoryear +\biblio_style plain +\use_bibtopic false +\use_indices false +\paperorientation portrait +\suppress_date false +\justification true +\use_refstyle 0 +\use_formatted_ref 0 +\use_minted 0 +\use_lineno 0 +\index Index +\shortcut idx +\color #008000 +\end_index +\secnumdepth 3 +\tocdepth 0 +\paragraph_separation indent +\paragraph_indentation default +\is_math_indent 0 +\math_numbering_side default +\quotes_style english +\dynamic_quotes 0 +\papercolumns 1 +\papersides 1 +\paperpagestyle default +\tablestyle default +\tracking_changes false +\output_changes false +\change_bars false +\postpone_fragile_content false +\html_math_output 0 +\html_css_as_file 0 +\html_be_strict false +\docbook_table_output 0 +\docbook_mathml_prefix 1 +\end_header + +\begin_body + +\begin_layout Standard +\begin_inset Note Note +status open + +\begin_layout Plain Layout +\noindent +\align left +Sample document for contributions to journals of the American Astronomical Society (AAS). + Please consult the +\begin_inset CommandInset href +LatexCommand href +name "AASTeX user guide" +target "http://journals.aas.org/authors/aastex/aasguide.html" +literal "false" + +\end_inset + + for details on how to use AASTeX. + +\end_layout + +\begin_layout Plain Layout +\noindent +\align left +An up-to-date sample LaTeX article using AASTeX is available under +\begin_inset Flex URL +status open + +\begin_layout Plain Layout + +http://journals.aas.org/authors/aastex/aastex.html#_download +\end_layout + +\end_inset + +. +\end_layout + +\end_inset + + +\begin_inset Note Note +status open + +\begin_layout Plain Layout +\noindent +\align left +The AASTeX document class uses a different name since version 6.0 (2016/02/16). + Depending on the version installed on your system, + set the document class to American Astronomical Society (AASTeX v. + 6) or American Astronomical Society (AASTeX v. + 5). + +\end_layout + +\begin_layout Plain Layout +\noindent +\align left +New features (cf. + +\begin_inset Flex URL +status collapsed + +\begin_layout Plain Layout + +http://journals.aas.org/authors/aastex/revisionhistory.html +\end_layout + +\end_inset + +) are only partially supported by LyX (see +\begin_inset Flex URL +status collapsed + +\begin_layout Plain Layout + +https://www.lyx.org/trac/ticket/10027 +\end_layout + +\end_inset + +). +\end_layout + +\end_inset + + +\end_layout + +\begin_layout Title +Collapsed Cores in Globular Clusters, + Gauge-Boson Couplings, + and AAS\SpecialChar TeX + Examples +\end_layout + +\begin_layout Author +S. + Djorgovski and Ivan R. + King +\end_layout + +\begin_layout Affiliation +Astronomy Department, + University of California, + Berkeley, + CA 94720 +\end_layout + +\begin_layout Altaffilation +Visiting Astronomer +\begin_inset Newline newline +\end_inset + + Cerro Tololo Inter-American Observatory. +\begin_inset Newline newline +\end_inset + +CTIO is operated by AURA Inc. +\begin_inset space \space{} +\end_inset + +under contract to the National Science Foundation. +\end_layout + +\begin_layout Altaffilation +Society of Fellows, + Harvard University. +\end_layout + +\begin_layout Altaffilation +present address: + Center for Astrophysics +\begin_inset Newline newline +\end_inset + +60 Garden Street, + Cambridge, + MA 02138 +\end_layout + +\begin_layout Author +C. + D. + Biemesderfer +\end_layout + +\begin_layout Affiliation +National Optical Astronomy Observatories, + Tucson, + AZ 85719 +\end_layout + +\begin_layout Altaffilation +Visiting Programmer, + Space Telescope Science Institute +\end_layout + +\begin_layout Altaffilation +Patron, + Alonso's Bar and Grill +\end_layout + +\begin_layout Email +aastex-help@aas.org +\end_layout + +\begin_layout Author +R. + J. + Hanisch +\end_layout + +\begin_layout Affiliation +Space Telescope Science Institute, + Baltimore, + MD 21218 +\end_layout + +\begin_layout Altaffilation +Patron, + Alonso's Bar and Grill +\end_layout + +\begin_layout Abstract +This is a preliminary report on surface photometry of the major fraction of known globular clusters, + to see which of them show the signs of a collapsed core. + We also explore some diversionary mathematics and recreational tables. + +\end_layout + +\begin_layout Keywords +clusters: + globular, + peanut— +bosons: + bozos +\end_layout + +\begin_layout Section +Introduction +\end_layout + +\begin_layout Standard +A focal problem today in the dynamics of globular clusters is core collapse. + It has been predicted by theory for decades +\begin_inset CommandInset citation +LatexCommand citep +key "hen61,lyn68,spi85" +literal "false" + +\end_inset + +, + but observation has been less alert to the phenomenon. + For many years the central brightness peak in M15 +\begin_inset CommandInset citation +LatexCommand citep +key "kin75,new78" +literal "false" + +\end_inset + + seemed a unique anomaly. + Then +\begin_inset CommandInset citation +LatexCommand citep +key "aur82" +literal "false" + +\end_inset + + suggested a central peak in NGC 6397, + and a limited photographic survey of ours +\begin_inset CommandInset citation +LatexCommand citep +after "Paper I" +key "djo84" +literal "false" + +\end_inset + + found three more cases, + including NGC 6624, + whose sharp center had often been remarked on +\begin_inset CommandInset citation +LatexCommand citep +key "can78" +literal "false" + +\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 CommandInset citation +LatexCommand citep +key "kin68,pet76,har84,ort85" +literal "false" + +\end_inset + +, + as well as photoelectric profiles +\begin_inset CommandInset citation +LatexCommand citep +key "kin66,kin75" +literal "false" + +\end_inset + + and electronographic profiles +\begin_inset CommandInset citation +LatexCommand citep +key "kro84" +literal "false" + +\end_inset + +. + In a few cases we judged normality by eye estimates on one of the Sky Surveys. +\end_layout + +\begin_layout Section +Helicity Amplitudes +\end_layout + +\begin_layout Standard +It has been realized that helicity amplitudes provide a convenient means for Feynman diagram +\begin_inset Foot +status collapsed + +\begin_layout Plain Layout +Footnotes can be inserted like this. +\end_layout + +\end_inset + + evaluations. + These amplitude-level techniques are particularly convenient for calculations involving many Feynman diagrams, + where the usual trace techniques for the amplitude squared becomes unwieldy. + Our calculations use the helicity techniques developed by other authors +\begin_inset CommandInset citation +LatexCommand cite +key "hag86" +literal "true" + +\end_inset + +; + we briefly summarize below. +\end_layout + +\begin_layout Subsection +Formalism +\end_layout + +\begin_layout Standard +\begin_inset CommandInset label +LatexCommand label +name "bozomath" + +\end_inset + + +\end_layout + +\begin_layout Standard +A tree-level amplitude in +\begin_inset Formula $e^{+}e^{-}$ +\end_inset + + collisions can be expressed in terms of fermion strings of the form +\begin_inset Formula +\begin{equation} +\bar{v}(p_{2},\sigma_{2})P_{-\tau}\hat{a}_{1}\hat{a}_{2}\cdots\hat{a}_{n}u(p_{1},\sigma_{1}), +\end{equation} + +\end_inset + + where +\begin_inset Formula $p$ +\end_inset + + and +\begin_inset Formula $\sigma$ +\end_inset + + label the initial +\begin_inset Formula $e^{\pm}$ +\end_inset + + four-momenta and helicities +\begin_inset Formula $(\sigma=\pm1)$ +\end_inset + +, + +\begin_inset Formula $\hat{a}_{i}=a_{i}^{\mu}\gamma_{\nu}$ +\end_inset + + and +\begin_inset Formula $P_{\tau}=\frac{1}{2}(1+\tau\gamma_{5})$ +\end_inset + + is a chirality projection operator +\begin_inset Formula $(\tau=\pm1)$ +\end_inset + +. + The +\begin_inset Formula $a_{i}^{\mu}$ +\end_inset + + may be formed from particle four-momenta, + gauge-boson polarization vectors or fermion strings with an uncontracted Lorentz index associated with final-state fermions. +\end_layout + +\begin_layout NoteToEditor +Figures 1 and 2 should appear side-by-side in print +\end_layout + +\begin_layout Standard +In the chiral representation the +\begin_inset Formula $\gamma$ +\end_inset + + matrices are expressed in terms of +\begin_inset Formula $2\times2$ +\end_inset + + Pauli matrices +\begin_inset Formula $\sigma$ +\end_inset + + and the unit matrix 1 as +\begin_inset Formula +\begin{eqnarray*} +\gamma^{\mu} & = & \left(\begin{array}{cc} +0 & \sigma_{+}^{\mu}\\ +\sigma_{-}^{\mu} & 0 +\end{array}\right),\gamma^{5}=\left(\begin{array}{cc} +-1 & 0\\ +0 & 1 +\end{array}\right),\\ +\sigma_{\pm}^{\mu} & = & (\textbf{1},\pm\sigma), +\end{eqnarray*} + +\end_inset + + giving +\begin_inset Formula +\begin{equation} +\hat{a}=\left(\begin{array}{cc} +0 & (\hat{a})_{+}\\ +(\hat{a})_{-} & 0 +\end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu}, +\end{equation} + +\end_inset + + The spinors are expressed in terms of two-component Weyl spinors as +\begin_inset Formula +\begin{equation} +u=\left(\begin{array}{c} +(u)_{-}\\ +(u)_{+} +\end{array}\right),v=\textbf{(}v_{+}^{\dagger}\textbf{,}v_{-}^{\dagger}\textbf{)}. +\end{equation} + +\end_inset + + +\end_layout + +\begin_layout Standard +The Weyl spinors are given in terms of helicity eigenstates +\begin_inset Formula $\chi_{\lambda}(p)$ +\end_inset + + with +\begin_inset Formula $\lambda=\pm1$ +\end_inset + + by +\end_layout + +\begin_layout MathLetters +\begin_inset Formula +\begin{eqnarray} +u(p,\lambda)_{\pm} & = & (E\pm\lambda|\textbf{p}|)^{1/2}\chi_{\lambda}(p),\\ +v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|\textbf{p}|)^{1/2}\chi_{-\lambda}(p) +\end{eqnarray} + +\end_inset + + +\end_layout + +\begin_layout Section +Floating material and so forth +\end_layout + +\begin_layout Standard +Consider a task that computes profile parameters for a modified Lorentzian of the form +\begin_inset Formula +\begin{equation} +I=\frac{1}{1+d_{1}^{P(1+d_{2})}} +\end{equation} + +\end_inset + + where +\begin_inset Formula +\[ +d_{1}=\sqrt{\left(\begin{array}{c} +\frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c} +\frac{y_{1}}{R_{min}}\end{array}\right)^{2}} +\] + +\end_inset + + +\begin_inset Formula +\[ +d_{2}=\sqrt{\left(\begin{array}{c} +\frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c} +\case{y_{1}}{PR_{min}}\end{array}\right)^{2}} +\] + +\end_inset + + +\begin_inset Formula +\[ +x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta +\] + +\end_inset + + +\begin_inset Formula +\[ +y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta +\] + +\end_inset + + +\end_layout + +\begin_layout Standard +In these expressions +\begin_inset Formula $x_{0}$ +\end_inset + +, +\begin_inset Formula $y_{0}$ +\end_inset + + is the star center, + and +\begin_inset Formula $\Theta$ +\end_inset + + is the angle with the +\begin_inset Formula $x$ +\end_inset + + axis. + Results of this task are shown in table +\begin_inset space ~ +\end_inset + + +\begin_inset CommandInset ref +LatexCommand ref +reference "tbl-2" +nolink "false" + +\end_inset + +. + It is not clear how these sorts of analyses may affect determination of +\begin_inset Formula $M_{\text{\sun}}$ +\end_inset + +, + but the assumption is that the alternate results should be less than 90° out of phase with previous values. + We have no observations of +\begin_inset Preview + +\begin_layout Standard +\begin_inset ERT +status open + +\begin_layout Plain Layout + + +\backslash +ion{Ca}{2} +\end_layout + +\end_inset + + +\end_layout + +\end_inset + +. + Roughly +\begin_inset Formula $\nicefrac{4}{5}$ +\end_inset + + of the electronically submitted abstracts for AAS meetings are error-free. + +\end_layout + +\begin_layout Acknowledgments +We are grateful to V. + Barger, + T. + Han, + and R. + J. + N. + Phillips for doing the math in section +\begin_inset space ~ +\end_inset + + +\begin_inset CommandInset ref +LatexCommand ref +reference "bozomath" +nolink "false" + +\end_inset + +. + More information on the AAS\SpecialChar TeX + macros package are available at +\begin_inset Flex URL +status collapsed + +\begin_layout Plain Layout + +http://www.aas.org/publications/aastex +\end_layout + +\end_inset + + or the +\begin_inset CommandInset href +LatexCommand href +name "AAS ftp site" +target "ftp://www.aas.org/pubs/AAS ftp site" +literal "false" + +\end_inset + +. +\end_layout + +\begin_layout Software +IRAF, + AIPS, + Astropy, + ... +\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 Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Auri\\`ere(1982)" +key "aur82" +literal "true" + +\end_inset + +Aurière, + M. + 1982, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +aap +\end_layout + +\end_inset + +, + 109, + 301 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Canizares et al.(1978)" +key "can78" +literal "true" + +\end_inset + +Canizares, + C. + R., + Grindlay, + J. + E., + Hiltner, + W. + A., + Liller, + W., + and McClintock, + J. + E. + 1978, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +apj +\end_layout + +\end_inset + +, + 224, + 39 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Djorgovski and King(1984)" +key "djo84" +literal "true" + +\end_inset + +Djorgovski, + S., + and King, + I. + R. + 1984, + +\begin_inset Preview + +\begin_layout Standard +\begin_inset ERT +status open + +\begin_layout Plain Layout + + +\backslash +apjl +\end_layout + +\end_inset + + +\end_layout + +\end_inset + +, + 277, + L49 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Hagiwara and Zeppenfeld(1986)" +key "hag86" +literal "true" + +\end_inset + +Hagiwara, + K., + and Zeppenfeld, + D. + 1986, + Nucl.Phys., + 274, + 1 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Harris and van den Bergh(1984)" +key "har84" +literal "true" + +\end_inset + +Harris, + W. + E., + and van den Bergh, + S. + 1984, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +aj +\end_layout + +\end_inset + +, + 89, + 1816 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "H\\`enon(1961)" +key "hen61" +literal "true" + +\end_inset + +Hénon, + M. + 1961, + Ann.d'Ap., + 24, + 369 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "King(1966)" +key "kin66" +literal "true" + +\end_inset + +King, + I. + R. + 1966, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +aj +\end_layout + +\end_inset + +, + 71, + 276 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "King(1975)" +key "kin75" +literal "true" + +\end_inset + +King, + I. + R. + 1975, + Dynamics of Stellar Systems, + A. + Hayli, + Dordrecht: + Reidel, + 1975, + 99 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "King et al.(1968)" +key "kin68" +literal "true" + +\end_inset + +King, + I. + R., + Hedemann, + E., + Hodge, + S. + M., + and White, + R. + E. + 1968, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +aj +\end_layout + +\end_inset + +, + 73, + 456 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Kron et al.(1984)" +key "kro84" +literal "true" + +\end_inset + +Kron, + G. + E., + Hewitt, + A. + V., + and Wasserman, + L. + H. + 1984, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +pasp +\end_layout + +\end_inset + +, + 96, + 198 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Lynden-Bell and Wood(1968)" +key "lyn68" +literal "true" + +\end_inset + +Lynden-Bell, + D., + and Wood, + R. + 1968, + +\begin_inset Preview + +\begin_layout Standard +\begin_inset ERT +status open + +\begin_layout Plain Layout + + +\backslash +mnras +\end_layout + +\end_inset + + +\end_layout + +\end_inset + +, + 138, + 495 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Newell and O'Neil(1978)" +key "new78" +literal "true" + +\end_inset + +Newell, + E. + B., + and O'Neil, + E. + J. + 1978, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +apjs +\end_layout + +\end_inset + +, + 37, + 27 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Ortolani et al.(1985)" +key "ort85" +literal "true" + +\end_inset + +Ortolani, + S., + Rosino, + L., + and Sandage, + A. + 1985, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +aj +\end_layout + +\end_inset + +, + 90, + 473 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Peterson(1976)" +key "pet76" +literal "true" + +\end_inset + +Peterson, + C. + J. + 1976, + +\begin_inset ERT +status collapsed + +\begin_layout Plain Layout + + +\backslash +aj +\end_layout + +\end_inset + +, + 81, + 617 +\end_layout + +\begin_layout Bibliography +\begin_inset CommandInset bibitem +LatexCommand bibitem +label "Spitzer(1985)" +key "spi85" +literal "true" + +\end_inset + +Spitzer, + L. + 1985, + Dynamics of Star Clusters, + J. + Goodman and P. + Hut, + Dordrecht: + Reidel, + 109 +\end_layout + +\begin_layout Standard +\begin_inset Newpage clearpage +\end_inset + + +\end_layout + +\begin_layout Standard +\begin_inset Caption FigCaption + +\begin_layout Plain Layout +\begin_inset 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-\begin_body - -\begin_layout Standard -\begin_inset Note Note -status open - -\begin_layout Plain Layout -\noindent -\align left -Sample document for contributions to journals of the American Astronomical Society (AAS). - Please consult the -\begin_inset CommandInset href -LatexCommand href -name "AASTeX user guide" -target "http://journals.aas.org/authors/aastex/aasguide.html" -literal "false" - -\end_inset - - for details on how to use AASTeX. - -\end_layout - -\begin_layout Plain Layout -\noindent -\align left -An up-to-date sample LaTeX article using AASTeX is available under -\begin_inset Flex URL -status open - -\begin_layout Plain Layout - -http://journals.aas.org/authors/aastex/aastex.html#_download -\end_layout - -\end_inset - -. -\end_layout - -\end_inset - - -\begin_inset Note Note -status open - -\begin_layout Plain Layout -\noindent -\align left -The AASTeX document class uses a different name since version 6.0 (2016/02/16). - Depending on the version installed on your system, - set the document class to American Astronomical Society (AASTeX v. - 6) or American Astronomical Society (AASTeX v. - 5). - -\end_layout - -\begin_layout Plain Layout -\noindent -\align left -New features (cf. - -\begin_inset Flex URL -status collapsed - -\begin_layout Plain Layout - -http://journals.aas.org/authors/aastex/revisionhistory.html -\end_layout - -\end_inset - -) are only partially supported by LyX (see -\begin_inset Flex URL -status collapsed - -\begin_layout Plain Layout - -https://www.lyx.org/trac/ticket/10027 -\end_layout - -\end_inset - -). -\end_layout - -\end_inset - - -\end_layout - -\begin_layout Title -Collapsed Cores in Globular Clusters, - Gauge-Boson Couplings, - and AAS\SpecialChar TeX - Examples -\end_layout - -\begin_layout Author -S. - Djorgovski and Ivan R. - King -\end_layout - -\begin_layout Affiliation -Astronomy Department, - University of California, - Berkeley, - CA 94720 -\end_layout - -\begin_layout Altaffilation -Visiting Astronomer -\begin_inset Newline newline -\end_inset - - Cerro Tololo Inter-American Observatory. -\begin_inset Newline newline -\end_inset - -CTIO is operated by AURA Inc. -\begin_inset space \space{} -\end_inset - -under contract to the National Science Foundation. -\end_layout - -\begin_layout Altaffilation -Society of Fellows, - Harvard University. -\end_layout - -\begin_layout Altaffilation -present address: - Center for Astrophysics -\begin_inset Newline newline -\end_inset - -60 Garden Street, - Cambridge, - MA 02138 -\end_layout - -\begin_layout Author -C. - D. - Biemesderfer -\end_layout - -\begin_layout Affiliation -National Optical Astronomy Observatories, - Tucson, - AZ 85719 -\end_layout - -\begin_layout Altaffilation -Visiting Programmer, - Space Telescope Science Institute -\end_layout - -\begin_layout Altaffilation -Patron, - Alonso's Bar and Grill -\end_layout - -\begin_layout Email -aastex-help@aas.org -\end_layout - -\begin_layout Author -R. - J. - Hanisch -\end_layout - -\begin_layout Affiliation -Space Telescope Science Institute, - Baltimore, - MD 21218 -\end_layout - -\begin_layout Altaffilation -Patron, - Alonso's Bar and Grill -\end_layout - -\begin_layout Abstract -This is a preliminary report on surface photometry of the major fraction of known globular clusters, - to see which of them show the signs of a collapsed core. - We also explore some diversionary mathematics and recreational tables. - -\end_layout - -\begin_layout Keywords -clusters: - globular, - peanut— -bosons: - bozos -\end_layout - -\begin_layout Section -Introduction -\end_layout - -\begin_layout Standard -A focal problem today in the dynamics of globular clusters is core collapse. - It has been predicted by theory for decades -\begin_inset CommandInset citation -LatexCommand citep -key "hen61,lyn68,spi85" -literal "false" - -\end_inset - -, - but observation has been less alert to the phenomenon. - For many years the central brightness peak in M15 -\begin_inset CommandInset citation -LatexCommand citep -key "kin75,new78" -literal "false" - -\end_inset - 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-. - The -\begin_inset Formula $a_{i}^{\mu}$ -\end_inset - - may be formed from particle four-momenta, - gauge-boson polarization vectors or fermion strings with an uncontracted Lorentz index associated with final-state fermions. -\end_layout - -\begin_layout NoteToEditor -Figures 1 and 2 should appear side-by-side in print -\end_layout - -\begin_layout Standard -In the chiral representation the -\begin_inset Formula $\gamma$ -\end_inset - - matrices are expressed in terms of -\begin_inset Formula $2\times2$ -\end_inset - - Pauli matrices -\begin_inset Formula $\sigma$ -\end_inset - - and the unit matrix 1 as -\begin_inset Formula -\begin{eqnarray*} -\gamma^{\mu} & = & \left(\begin{array}{cc} -0 & \sigma_{+}^{\mu}\\ -\sigma_{-}^{\mu} & 0 -\end{array}\right),\gamma^{5}=\left(\begin{array}{cc} --1 & 0\\ -0 & 1 -\end{array}\right),\\ -\sigma_{\pm}^{\mu} & = & (\textbf{1},\pm\sigma), -\end{eqnarray*} - -\end_inset - - giving -\begin_inset Formula -\begin{equation} -\hat{a}=\left(\begin{array}{cc} -0 & (\hat{a})_{+}\\ -(\hat{a})_{-} & 0 -\end{array}\right),(\hat{a})_{\pm}=a_{\mu}\sigma_{\pm}^{\mu}, -\end{equation} - -\end_inset - - The spinors are expressed in terms of two-component Weyl spinors as -\begin_inset Formula -\begin{equation} -u=\left(\begin{array}{c} -(u)_{-}\\ -(u)_{+} -\end{array}\right),v=\textbf{(}v_{+}^{\dagger}\textbf{,}v_{-}^{\dagger}\textbf{)}. -\end{equation} - -\end_inset - - -\end_layout - -\begin_layout Standard -The Weyl spinors are given in terms of helicity eigenstates -\begin_inset Formula $\chi_{\lambda}(p)$ -\end_inset - - with -\begin_inset Formula $\lambda=\pm1$ -\end_inset - - by -\end_layout - -\begin_layout MathLetters -\begin_inset Formula -\begin{eqnarray} -u(p,\lambda)_{\pm} & = & (E\pm\lambda|\textbf{p}|)^{1/2}\chi_{\lambda}(p),\\ -v(p,\lambda)_{\pm} & = & \pm\lambda(E\mp\lambda|\textbf{p}|)^{1/2}\chi_{-\lambda}(p) -\end{eqnarray} - -\end_inset - - -\end_layout - -\begin_layout Section -Floating material and so forth -\end_layout - -\begin_layout Standard -Consider a task that computes profile parameters for a modified Lorentzian of the form -\begin_inset Formula -\begin{equation} -I=\frac{1}{1+d_{1}^{P(1+d_{2})}} -\end{equation} - -\end_inset - - where -\begin_inset Formula -\[ -d_{1}=\sqrt{\left(\begin{array}{c} -\frac{x_{1}}{R_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c} -\frac{y_{1}}{R_{min}}\end{array}\right)^{2}} -\] - -\end_inset - - -\begin_inset Formula -\[ -d_{2}=\sqrt{\left(\begin{array}{c} -\frac{x_{1}}{PR_{maj}}\end{array}\right)^{2}+\left(\begin{array}{c} -\case{y_{1}}{PR_{min}}\end{array}\right)^{2}} -\] - -\end_inset - - -\begin_inset Formula -\[ -x_{1}=(x-x_{0})\cos\Theta+(y-y_{0})\sin\Theta -\] - -\end_inset - - -\begin_inset Formula -\[ -y_{1}=-(x-x_{0})\sin\Theta+(y-y_{0})\cos\Theta -\] - -\end_inset - - -\end_layout - -\begin_layout Standard -In these expressions -\begin_inset Formula $x_{0}$ -\end_inset - -, -\begin_inset Formula $y_{0}$ -\end_inset - - is the star center, - and -\begin_inset Formula $\Theta$ -\end_inset - - is the angle with the -\begin_inset Formula $x$ -\end_inset - - axis. - Results of this task are shown in table -\begin_inset space ~ -\end_inset - - -\begin_inset CommandInset ref -LatexCommand ref -reference "tbl-2" -nolink "false" - -\end_inset - -. - It is not clear how these sorts of analyses may affect determination of -\begin_inset Formula $M_{\text{\sun}}$ -\end_inset - -, - but the assumption is that the alternate results should be less than 90° out of phase with previous values. - We have no observations of -\begin_inset Preview - -\begin_layout Standard -\begin_inset ERT -status open - -\begin_layout Plain Layout - - -\backslash -ion{Ca}{2} -\end_layout - -\end_inset - - -\end_layout - -\end_inset - -. - Roughly -\begin_inset Formula $\nicefrac{4}{5}$ -\end_inset - - of the electronically submitted abstracts for AAS meetings are error-free. - -\end_layout - -\begin_layout Acknowledgments -We are grateful to V. - Barger, - T. - Han, - and R. - J. - N. - Phillips for doing the math in section -\begin_inset space ~ -\end_inset - - -\begin_inset CommandInset ref -LatexCommand ref -reference "bozomath" -nolink "false" - -\end_inset - -. - More information on the AAS\SpecialChar TeX - macros package are available at -\begin_inset Flex URL -status collapsed - -\begin_layout Plain Layout - -http://www.aas.org/publications/aastex -\end_layout - -\end_inset - - or the -\begin_inset CommandInset href -LatexCommand href -name "AAS ftp site" -target "ftp://www.aas.org/pubs/AAS ftp site" -literal "false" - -\end_inset - -. -\end_layout - -\begin_layout Software -IRAF, - AIPS, - Astropy, - ... -\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 Bibliography -\begin_inset CommandInset bibitem -LatexCommand bibitem -label "Auri\\`ere(1982)" -key "aur82" -literal "true" - -\end_inset - -Aurière, - M. - 1982, - -\begin_inset ERT -status collapsed - -\begin_layout Plain Layout - - -\backslash -aap -\end_layout - -\end_inset - -, - 109, - 301 -\end_layout - -\begin_layout Bibliography -\begin_inset CommandInset bibitem -LatexCommand bibitem -label "Canizares et al.(1978)" -key "can78" -literal "true" - -\end_inset - -Canizares, - C. - R., - Grindlay, - J. - E., - Hiltner, - W. - A., - Liller, - W., - and McClintock, - J. - E. - 1978, - -\begin_inset ERT -status collapsed - 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class +\float_alignment class +\paperfontsize default +\spacing single +\use_hyperref false +\papersize default +\use_geometry false +\use_package amsmath 1 +\use_package amssymb 1 +\use_package cancel 1 +\use_package esint 1 +\use_package mathdots 1 +\use_package mathtools 1 +\use_package mhchem 1 +\use_package stackrel 1 +\use_package stmaryrd 1 +\use_package undertilde 1 +\cite_engine natbib +\cite_engine_type authoryear +\biblio_style plainnat +\use_bibtopic false +\use_indices false +\paperorientation portrait +\suppress_date false +\justification true +\use_refstyle 0 +\use_formatted_ref 0 +\use_minted 0 +\use_lineno 0 +\index Index +\shortcut idx +\color #008000 +\end_index +\secnumdepth 3 +\tocdepth 0 +\paragraph_separation indent +\paragraph_indentation default +\is_math_indent 0 +\math_numbering_side default +\quotes_style english +\dynamic_quotes 0 +\papercolumns 1 +\papersides 1 +\paperpagestyle default +\tablestyle default +\tracking_changes false +\output_changes false 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