<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE dataset SYSTEM "http://tarantella.gsfc.nasa.gov/xml/dataset_048.dtd">
<dataset subject="astronomy" xmlns:xlink="http://www.w3.org/XML/XLink/0.9">
	<title>The Spatial Distribution of Young Stars in Vela</title>
	<altname type="ADC">2020</altname>
		<altname type="CDS">II/20</altname>
		<altname type="brief">UBV Photometry of O &amp; B Stars in Vela</altname>
	<reference>
		<source>
<journal>
	<title>The Spatial Distribution of Young Stars in Vela</title>
	<author>
			<initial>J</initial>
			<lastName>Denoyelle</lastName></author>
	<name>Astron.  Astrophys. Suppl. Ser.</name>
	<volume>27</volume>
	<pageno>343</pageno>
		<date>
			<year>1977</year></date>
	<bibcode>1977A&amp;AS...27..343D</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Reddening.html">Reddening</keyword>
			<keyword xlink:href="Photometry_UBV.html">Photometry, UBV</keyword>
			<keyword xlink:href="Colors.html">Colors</keyword>
			<keyword xlink:href="Stars_OB.html">Stars, OB</keyword></keywords>
	<descriptions>
				<description>
				<para>
    Photoelectric UBV values, derived from observations made at the Boyden
    and  ESO observatories, are presented for  358 early-type stars in the
    Vela section of the southern Milky Way.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="data.dat">
	<title>Data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>rec</name>
			<definition>Record number (if several records for star)</definition>
			<units>---</units></field>
		<field>
			<name>Seq</name>
			<definition>Running number</definition>
			<units>---</units></field>
		<field>
			<name>HD</name>
			<definition>HD number</definition>
			<units>---</units></field>
		<field>
			<name>CPD</name>
			<definition>Cape Photographic Durch. (or CD)</definition>
			<units>---</units></field>
		<field>
			<name>n_CPD</name>
			<definition>* = CPDzone,num are from Cordoba Durch.</definition>
			<units>---</units></field>
		<field>
			<name>RAh</name>
			<definition>Right Ascension (1950) hours</definition>
			<units>h</units></field>
		<field>
			<name>RAm</name>
			<definition>Right Ascension (1950) minutes</definition>
			<units>min</units></field>
		<field>
			<name>DE-</name>
			<definition>Declination (1950) sign</definition>
			<units>---</units></field>
		<field>
			<name>DEd</name>
			<definition>Declination (1950) degrees</definition>
			<units>deg</units></field>
		<field>
			<name>DEm</name>
			<definition>Declination (1950) arcminutes</definition>
			<units>arcmin</units></field>
		<field>
			<name>GLON</name>
			<definition>Galactic longitude</definition>
			<units>deg</units></field>
		<field>
			<name>GLAT</name>
			<definition>Galactic latitude</definition>
			<units>deg</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude
	<footnote>
			<para>
   99.99 indicates that the datum is missing.</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>u_Vmag</name>
			<definition>Uncertainty flag for V</definition>
			<units>---</units></field>
		<field>
			<name>B-V</name>
			<definition>(B-V) color index</definition>
			<units>mag</units></field>
		<field>
			<name>u_B-V</name>
			<definition>Uncertainty flag for B-V</definition>
			<units>---</units></field>
		<field>
			<name>U-B</name>
			<definition>(U-B) color index</definition>
			<units>mag</units></field>
		<field>
			<name>u_U-B</name>
			<definition>Uncertainty flag for U-B</definition>
			<units>---</units></field>
		<field>
			<name>Sp</name>
			<definition>MK or HD spectral classification</definition>
			<units>---</units></field>
		<field>
			<name>ref</name>
			<definition>Number of the source for MK Dp.</definition>
			<units>---</units></field>
		<field>
			<name>Emission</name>
			<definition>E = Halpha emission noted on red plates</definition>
			<units>---</units></field>
		<field>
			<name>Sp2</name>
			<definition>Spectral type obtained from Q method</definition>
			<units>---</units></field>
		<field>
			<name>Q</name>
			<definition>Q parameter
	<footnote>
			<para>
  Q = (U-B) - 0.72 (B-V)</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>E(B-V)</name>
			<definition>(B-V) colour excess</definition>
			<units>mag</units></field>
		<field>
			<name>A(V)</name>
			<definition>A(V) parameter
	<footnote>
			<para>
  A(V) = 3 x E(B-V)</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>m-M</name>
			<definition>Distance modulus</definition>
			<units>mag</units></field>
		<field>
			<name>R</name>
			<definition>Distance of the star</definition>
			<units>pc</units></field>
		<field>
			<name>Z</name>
			<definition>Distance from the galactic plane
	<footnote>
			<para>
  Z = R*sin(GLAT)
</para></footnote></definition>
			<units>pc</units></field>
		<field>
			<name>Nobs</name>
			<definition>Number of observations</definition>
			<units>---</units></field>
		<field>
			<name>rem</name>
			<definition>* = Comment exists for this star</definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Julie Anne Watko</lastName>
				<affiliation>SSDOO/ADC</affiliation></creator>
	<date>
		<year>1996</year><month>May</month><day>24</day></date></ingest>
		</history>
	<identifier>II_20.xml</identifier></dataset>
