<?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>Line Blocking and equivalent widths in the spectrum of Pollux</title>
	<altname type="ADC">J/A+AS/42/391</altname>
		<altname type="CDS">J/A+AS/42/391</altname>
		<altname type="brief">Line Blocking and equivalent widths in the spectrum</altname>
	<reference>
		<source>
<journal>
	<title>Line Blocking and equivalent widths in the spectrum of Pollux</title>
	<author>
			<initial>F</initial>
			<lastName>Ruland</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Griffin</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Griffin</lastName></author>
	<author>
			<initial>D</initial>
			<lastName>Biehl</lastName></author>
	<author>
			<initial>H</initial>
			<lastName>Holweger</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>42</volume>
	<pageno>391</pageno>
		<date>
			<year>1980</year></date>
	<bibcode>1980A&amp;AS...42..391R</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="spectroscopy.html">spectroscopy</keyword>
			<keyword xlink:href="stars_late-type.html">stars: late-type</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   High-dispersion spectrograms of Pollux (beta Gem, K0III) have been
   used to derive line blocking coeffecients for the spectral range
   4900-9300 A, and equivalent widths of lines of 43 atoms, ions, and molecules.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Equivalent widths of atomic and ionic lines
                                 measured from the spectrum of Pollux.</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Lambda</name>
			<definition>Wavelength in Angstroem</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Ion</name>
			<definition>Ion designation</definition>
			<units>---</units></field>
		<field>
			<name>Mult</name>
			<definition>Multiplet number</definition>
			<units>---</units></field>
		<field>
			<name>W</name>
			<definition>Equivalent width of line in Pollux
                                    in milliAngstroem</definition>
			<units>0.1pm</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3">
	<title>Equivalent widths of molecular lines in Pollux</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Lambda</name>
			<definition>Wavelength in Angstroem</definition>
			<units>0.1nm</units></field>
		<field>
			<name>Mol</name>
			<definition>Molecule designation</definition>
			<units>---</units></field>
		<field>
			<name>W</name>
			<definition>Equivalent width of line in Pollux
                                  in milliAngstroem</definition>
			<units>0.1pm</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>M.J. Wagner,   Francois Ochsenbein</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1993</year><month>Jul</month><day>27</day></date></ingest>
		</history>
	<identifier>J_A+AS_42_391.xml</identifier></dataset>
