<?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 Barium stars in the Hertzsprung-Russell diagram</title>
	<altname type="ADC">J/A+A/321/L9</altname>
		<altname type="CDS">J/A+A/321/L9</altname>
		<altname type="brief">Barium stars in the HR diagram</altname>
	<reference>
		<source>
<other>
	<title>The Barium stars in the Hertzsprung-Russell diagram</title>
	<author>
			<initial>J</initial>
			<lastName>Bergeat</lastName></author>
	<author>
			<initial>A</initial>
			<lastName>Knapik</lastName></author>
	<name>Astron. Astrophys. 321, L9</name>
	<publisher>???</publisher>
	<city>???</city>
	
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;A...321L...9B</bibcode></other></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Magnitudes_absolute.html">Magnitudes, absolute</keyword>
			<keyword xlink:href="Stars_barium.html">Stars, barium</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="Hertzsprung-Russell_(HR_diagram).html">Hertzsprung-Russell (HR diagram)</keyword>
			<keyword xlink:href="stars_chemically_peculiar.html">stars: chemically peculiar</keyword>
			<keyword xlink:href="stars_evolution.html">stars: evolution</keyword></keywords>
	<descriptions>
				<description>
				<para>
    Table2 is an extension of Table 1 to 15 additional stars with
    slightly less accurate parallaxes (see text). The entries are the same
    in both tables.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>The data for 37 Ba stars</title></tableLink>
				<tableLink xlink:href="table2">
	<title>The data for 15 Ba stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>HD</name>
			<definition>Henry Draper Catalogue (Cat. &lt;III/135>) or
                                   Lu (1991, Cat. &lt;V/81>) entry</definition>
			<units>---</units></field>
		<field>
			<name>G</name>
			<definition>Spectral group (see Sect. 2 of paper)</definition>
			<units>---</units></field>
		<field>
			<name>E(B-V)</name>
			<definition>Colour excess of interstellar extinction</definition>
			<units>mag</units></field>
		<field>
			<name>Mvl</name>
			<definition>Lower estimate of Mv</definition>
			<units>mag</units></field>
		<field>
			<name>Mv</name>
			<definition>Absolute visual magnitude
	<footnote footnoteId="???"><para>number=1</para>
			<para>Absolute visual magnitude between the lower and upper estimates
           as derived in Sect. 3</para></footnote></definition>
			<units>mag</units></field>
		<field>
			<name>Mvu</name>
			<definition>Upper estimate of Mv</definition>
			<units>mag</units></field>
		<field>
			<name>LumClass</name>
			<definition>Proposed luminosity class
	<footnote footnoteId="???"><para>number=2</para>
			<para>Proposed luminosity class (Sect. 4).
          III   = IIIab
          II-   : possibly IIIa
          IIIa- : possibly III
          IIIb- : possibly IVa
          IVb-  : possibly Va
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="tables.tex"><name>tables.tex</name><description><para>LaTeX version of the tables</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>J. Bergeat</lastName>
				<affiliation>CRAL-Observatoire de Lyon</affiliation></creator>
	<date>
		<year>1997</year><month>Mar</month><day>28</day></date><acknowledgement>Jacques Bergeat &lt;jb@image.univ-lyon1.fr></acknowledgement></ingest>
		</history>
	<identifier>J_A+A_321_L9.xml</identifier></dataset>
