<?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>Mass-luminosity relation of low-mass stars</title>
	<altname type="ADC">J/A+A/320/79</altname>
		<altname type="CDS">J/A+A/320/79</altname>
		<altname type="brief">Mass-luminosity relation of low-mass stars</altname>
	<reference>
		<source>
<journal>
	<title>Mass-luminosity relation of low-mass stars</title>
	<author>
			<initial>O</initial>
			<initial>Yu</initial>
			<lastName>Malkov</lastName></author>
	<author>
			<initial>A</initial>
			<initial>E</initial>
			<lastName>Piskunov</lastName></author>
	<author>
			<initial>D</initial>
			<initial>A</initial>
			<lastName>Shpil'kina</lastName></author>
	<name>Astron. Astrophys.</name>
	<volume>320</volume>
	<pageno>79</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;A...320...79M</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Stars_late-type.html">Stars, late-type</keyword>
			<keyword xlink:href="Stars_masses.html">Stars, masses</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="stars_late-type.html">stars: late-type</keyword>
			<keyword xlink:href="stars_low-mass_brown_dwarfs.html">stars: low-mass, brown dwarfs</keyword>
			<keyword xlink:href="stars_luminosity_function_mass_function.html">stars: luminosity function, mass function</keyword></keywords>
	<descriptions>
				<description>
				<para>
    To construct the MLR, empirical data for 56 stars in 30 low mass
    multiple systems, main sequence components of spectral class M0 and
    later were collected and processed. We considered only those systems
    where the determination of dynamical masses of components is possible,
    that is, where masses are derived directly from celestial mechanical
    considerations rather than from relations between mass and some
    observational parameter.</para></description>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2.dat">
	<title>Systems data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>GJ</name>
			<definition>Gliese &amp; Jahreiss (GJ) &lt;V/70> nomenclature
                                     from Preliminary Version of the Third
                                     Catalogue of Nearby Stars.</definition>
			<units>---</units></field>
		<field>
			<name>n_GJ</name>
			<definition>a: systems that have no GJ names</definition>
			<units>---</units></field>
		<field>
			<name>Plx</name>
			<definition>Parallax</definition>
			<units>arcsec</units></field>
		<field>
			<name>e_Plx</name>
			<definition>Parallax accuracy</definition>
			<units>arcsec</units></field>
		<field>
			<name>Per</name>
			<definition>Period
	<footnote footnoteId="???"><para>number=1</para>
			<para>Data is present when used for the mass calculation, otherwise blank
</para></footnote></definition>
			<units>yr</units></field>
		<field>
			<name>e_Per</name>
			<definition>Period accuracy
	<footnote footnoteId="???"><para>number=1</para>
			<para>Data is present when used for the mass calculation, otherwise blank
</para></footnote></definition>
			<units>yr</units></field>
		<field>
			<name>a</name>
			<definition>Semimajor axis
	<footnote footnoteId="???"><para>number=1</para>
			<para>Data is present when used for the mass calculation, otherwise blank
</para></footnote></definition>
			<units>arcsec</units></field>
		<field>
			<name>e_a</name>
			<definition>Semimajor axis accuracy
	<footnote footnoteId="???"><para>number=1</para>
			<para>Data is present when used for the mass calculation, otherwise blank
</para></footnote></definition>
			<units>arcsec</units></field>
		<field>
			<name>Mass</name>
			<definition>Fractional mass of the secondary
	<footnote footnoteId="???"><para>number=1</para>
			<para>Data is present when used for the mass calculation, otherwise blank
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>e_Mass</name>
			<definition>Fractional mass accuracy
	<footnote footnoteId="???"><para>number=1</para>
			<para>Data is present when used for the mass calculation, otherwise blank
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Refs</name>
			<definition>References detailed in file "refs.dat"</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table4.dat">
	<title>Components data</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>GJ</name>
			<definition>Gliese &amp; Jahreiss (GJ) &lt;V/70> nomenclature
                                      from Preliminary Version of the Third
                                     Catalogue of Nearby Stars.</definition>
			<units>---</units></field>
		<field>
			<name>n_GJ</name>
			<definition>a: systems that have no GJ names</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>Visual stellar magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Vmag</name>
			<definition>Visual stellar magnitude accuracy</definition>
			<units>mag</units></field>
		<field>
			<name>flareFlag</name>
			<definition>* indicating flare stars</definition>
			<units>---</units></field>
		<field>
			<name>BolCorr</name>
			<definition>Bolometric correction (if known)</definition>
			<units>mag</units></field>
		<field>
			<name>e_BolCorr</name>
			<definition>Bolometric correction accuracy (if known)</definition>
			<units>mag</units></field>
		<field>
			<name>M(Vmag)</name>
			<definition>Absolute stellar magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_M(Vmag)</name>
			<definition>Absolute stellar magnitude accuracy</definition>
			<units>mag</units></field>
		<field>
			<name>log(L)</name>
			<definition>Bolometric luminosity (if known)</definition>
			<units>[solLum]</units></field>
		<field>
			<name>e_log(L)</name>
			<definition>Bolometric luminosity accuracy (if known)</definition>
			<units>[solLum]</units></field>
		<field>
			<name>Mass</name>
			<definition>Mass</definition>
			<units>solMass</units></field>
		<field>
			<name>e_Mass</name>
			<definition>Mass accuracy</definition>
			<units>solMass</units></field>
		<field>
			<name>Note2</name>
			<definition>+ indicating stars with the best data</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="refs.dat">
	<title>References of table2</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>RefNo</name>
			<definition>Reference number</definition>
			<units>---</units></field>
		<field>
			<name>---</name>
			<definition>Separator</definition>
			<units>---</units></field>
		<field>
			<name>Text</name>
			<definition>Name of author(s), and bibcode</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>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1996</year><month>Oct</month><day>07</day></date></ingest>
		</history>
	<identifier>J_A+A_320_79.xml</identifier></dataset>
