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authorJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
committerJoseph Hunkeler <jhunkeler@gmail.com>2015-03-04 21:21:30 -0500
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treeafc52015ffc2c74e0266653eecef1c8ef8ba5d91 /src/slalib/sun67.htx/node171.html
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+<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 3.2//EN">
+<!--Converted with LaTeX2HTML 97.1 (release) (July 13th, 1997)
+ by Nikos Drakos (nikos@cbl.leeds.ac.uk), CBLU, University of Leeds
+* revised and updated by: Marcus Hennecke, Ross Moore, Herb Swan
+* with significant contributions from:
+ Jens Lippman, Marek Rouchal, Martin Wilck and others -->
+<HTML>
+<HEAD>
+<TITLE>SLA_RVGALC - RV Corrn to Galactic Centre</TITLE>
+<META NAME="description" CONTENT="SLA_RVGALC - RV Corrn to Galactic Centre">
+<META NAME="keywords" CONTENT="sun67">
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+<BR>
+<B>Up:</B> <A NAME="tex2html2135" HREF="node13.html">SUBPROGRAM SPECIFICATIONS</A>
+<BR>
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+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<H2><A NAME="SECTION0004158000000000000000">SLA_RVGALC - RV Corrn to Galactic Centre</A>
+<A NAME="xref_SLA_RVGALC">&#160;</A><A NAME="SLA_RVGALC">&#160;</A>
+</H2>
+ <DL>
+<DT><STRONG>ACTION:</STRONG>
+<DD>Velocity component in a given direction due to the rotation
+of the Galaxy.
+<P> <DT><STRONG>CALL:</STRONG>
+<DD><TT>R&nbsp;=&nbsp;sla_RVGALC (R2000, D2000)</TT>
+<P> </DL>
+<P> <DL>
+<DT><STRONG>GIVEN:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>R2000,D2000</EM></TD>
+<TH ALIGN="LEFT"><B>R</B></TH>
+<TD ALIGN="LEFT" NOWRAP>J2000.0 mean <IMG WIDTH="42" HEIGHT="29" ALIGN="MIDDLE" BORDER="0"
+ SRC="img3.gif"
+ ALT="$[\,\alpha,\delta\,]$"> (radians)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>RETURNED:</STRONG>
+<DD>
+<BR>
+<TABLE CELLPADDING=3>
+<TR VALIGN="TOP"><TD ALIGN="LEFT"><EM>sla_RVGALC</EM></TD>
+<TH ALIGN="LEFT"><B>R</B></TH>
+<TD ALIGN="LEFT" NOWRAP>Component of dynamical LSR motion in direction
+R2000,D2000 (km&nbsp;s<SUP>-1</SUP>)</TD>
+</TR>
+</TABLE></DL>
+<P> <DL>
+<DT><STRONG>NOTES:</STRONG>
+<DD><DL COMPACT>
+<DT>1.
+<DD>Sign convention: the result is positive when the LSR
+is receding from the given point on the sky.
+<DT>2.
+<DD>The Local Standard of Rest used here is a point in the
+ vicinity of the Sun which is in a circular orbit around
+ the Galactic centre. Sometimes called the <I>dynamical</I> LSR,
+ it is not to be confused with a <I>kinematical</I> LSR, which
+ is the mean standard of rest of star catalogues or stellar
+ populations.
+ <DT>3.
+<DD>The dynamical LSR velocity due to Galactic rotation is assumed to
+ be 220&nbsp;km&nbsp;s<SUP>-1</SUP> towards <IMG WIDTH="64" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
+ SRC="img222.gif"
+ ALT="$l^{I\!I}=90^{\circ}$">, <IMG WIDTH="51" HEIGHT="17" ALIGN="BOTTOM" BORDER="0"
+ SRC="img223.gif"
+ ALT="$b^{I\!I}=0$">. </DL></DL>
+<P> <DL>
+<DT><STRONG>REFERENCE:</STRONG>
+<DD>Kerr &amp; Lynden-Bell (1986), MNRAS, 221, p1023.
+</DL>
+<BR> <HR>
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+<BR>
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+<BR>
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+<BR> <HR> <P>
+<P><!--End of Navigation Panel-->
+<ADDRESS>
+<I>SLALIB --- Positional Astronomy Library<BR>Starlink User Note 67<BR>P. T. Wallace<BR>12 October 1999<BR>E-mail:ptw@star.rl.ac.uk</I>
+</ADDRESS>
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+</HTML>