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- Velocity component in a given direction due to the Sun's motion with respect to the dynamical Local Standard of Rest
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<H2><A NAME="SECTION000465000000000000000"></A><A NAME="____palRvlsrd_"></A>
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palRvlsrd
palRvlsrd
- Velocity component in a given direction due to the Sun<TT>'</TT>s motion
with respect to the dynamical Local Standard of Rest
</H2>
<DL>
<DT><STRONG>Description:</STRONG></DT>
<DD><DL>
<DD>This function returns the velocity component in a given direction
due to the Sun<TT>'</TT>s motion with respect to the dynamical Local Standard
of Rest. The result is <SPAN CLASS="MATH"><IMG
WIDTH="18" HEIGHT="31" ALIGN="MIDDLE" BORDER="0"
SRC="img2.png"
ALT="$+$"></SPAN>ve when the Sun is receding from the given
point on the sky.
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Invocation:</STRONG></DT>
<DD><DL>
<DD><TT> double palRvlsrd( double r2000, double d2000 )
</TT>
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Arguments:</STRONG></DT>
<DD>
<BR> <DL>
<DT><STRONG>
r2000 = double (Given)
</STRONG></DT>
<DD>
J2000.0 mean RA (radians)
</DD>
<DT><STRONG>
d2000 = double (Given)
</STRONG></DT>
<DD>
J2000.0 mean Dec (radians)
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Returned Value:</STRONG></DT>
<DD>
<BR> <DL>
<DT><STRONG>
Component of <TT>"</TT>peculiar<TT>"</TT> solar motion in direction R2000,D2000 (km/s).
</STRONG></DT>
<DD>
</DD>
</DL>
<BR>
</DD>
<DT><STRONG>Notes:</STRONG></DT>
<DD><UL>
<LI>The Local Standard of Rest used here is the <TT>"</TT>dynamical<TT>"</TT> LSR,
a point in the vicinity of the Sun which is in a circular orbit
around the Galactic centre. The Sun<TT>'</TT>s motion with respect to the
dynamical LSR is called the <TT>"</TT>peculiar<TT>"</TT> solar motion.
<P>
</LI>
<LI>There is another type of LSR, called a <TT>"</TT>kinematical<TT>"</TT> LSR. A
kinematical LSR is the mean standard of rest of specified star
catalogues or stellar populations, and several slightly different
kinematical LSRs are in use. The Sun<TT>'</TT>s motion with respect to an
agreed kinematical LSR is known as the <TT>"</TT>standard<TT>"</TT> solar motion.
To obtain a radial velocity correction with respect to an adopted
kinematical LSR use the routine sla_RVLSRK.
</LI>
</UL>
<BR>
</DD>
<DT><STRONG>
Reference
</STRONG></DT>
<DD><UL>
<LI>Delhaye (1965), in <TT>"</TT>Stars and Stellar Systems<TT>"</TT>, vol 5, p73.
</LI>
</UL>
<BR>
</DD>
</DL>
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