<?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>Low resolution IUE spectra of Wolf-Rayet stars.</title>
	<altname type="ADC">J/A+AS/108/669</altname>
		<altname type="CDS">J/A+AS/108/669</altname>
		<altname type="brief">IUE spectra of WR stars</altname>
	<reference>
		<source>
<journal>
	<title>Low resolution IUE spectra of Wolf-Rayet stars.</title>
	<author>
			<initial>A</initial>
			<lastName>Niedzielski</lastName></author>
	<author>
			<initial>K</initial>
			<lastName>Rochowicz</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>108</volume>
	<pageno>669</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994A&amp;AS..108..669N</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="atlases.html">atlases</keyword>
			<keyword xlink:href="stars_classification.html">stars: classification</keyword>
			<keyword xlink:href="stars_Wolf-Rayet.html">stars: Wolf-Rayet</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   We present uniformly reduced and measured equivalent widths, FWHM and
   observed line fluxes for 94 "single" WR stars (34 galactic WN, 22 galactic
   WC, 31 LMC WN and 7 LMC WC) based on the archive IUE spectra of WR stars
   gathered from different observational runs and from different epochs. The
   spectra are used for spectral classification in the ultraviolet region and
   for searching correlations among the strength and widths of emission lines
   of different ions. Some correlations with optical and near IR lines
   observed by other authors are given as well. The set of spectra we use is
   almost complete to 12 magnitude and representative according to spectral
   subtype of WR stars.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table6">
	<title>Low resolution IUE spectra</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Gal</name>
			<definition>Star membership, galaxy or LMC</definition>
			<units>---</units></field>
		<field>
			<name>Type</name>
			<definition>Star type, WN or WC</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>Line</name>
			<definition>Identification observed wavelength</definition>
			<units>0.1nm</units></field>
		<field>
			<name>LogW</name>
			<definition>Equivalent width</definition>
			<units>0.1nm</units></field>
		<field>
			<name>FWHM</name>
			<definition>Full width at half maximum</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Flux</name>
			<definition>Observed (reddened) flux in a line</definition>
			<units>10mW/m2/nm</units></field></fields></tableHead>
	
			<textFile xlink:href="tabwcg.tex"><name>tabwcg.tex</name><description><para>LaTeX version of table6 for galactic WC stars</para></description></textFile>
			<textFile xlink:href="tabwcl.tex"><name>tabwcl.tex</name><description><para>LaTeX version of table6 for LMC WC stars</para></description></textFile>
			<textFile xlink:href="tabwng.tex"><name>tabwng.tex</name><description><para>LaTeX version of table6 for galactic WN stars</para></description></textFile>
			<textFile xlink:href="tabwnl.tex"><name>tabwnl.tex</name><description><para>LaTeX version of table6 for LMC WC stars</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Sep</month><day>19</day></date></ingest>
		</history>
	<identifier>J_A+AS_108_669.xml</identifier></dataset>
