<?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 light variations of some CP2 SrCrEu</title>
	<altname type="ADC">J/A+AS/108/595</altname>
		<altname type="CDS">J/A+AS/108/595</altname>
		<altname type="brief">CP2 SrCrEu stars light variation</altname>
	<reference>
		<source>
<journal>
	<title>The light variations of some CP2 SrCrEu</title>
	<author>
			<initial>F</initial>
			<initial>A</initial>
			<lastName>Catalano</lastName></author>
	<author>
			<initial>F</initial>
			<lastName>Leone</lastName></author>
	<name>Astron. Astrophys. Suppl. Ser.</name>
	<volume>108</volume>
	<pageno>595</pageno>
		<date>
			<year>1994</year></date>
	<bibcode>1994A&amp;AS..108..595C</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="stars_chemically_peculiar.html">stars: chemically peculiar</keyword>
			<keyword xlink:href="stars_variables_other.html">stars: variables: other</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   In the framework of a programme of checking the periods of chemically
   peculiar stars, eight southern stars have been observed in the uvby system.
   Seven stars have been previously known to be light variables, but for some
   stars the periods were not accurate enough to phase together different kinds
   of observations carried out several years apart. The periods of HD 83368,
   HD 98088, and HD 153882 are confirmed. For the stars HD 49976, HD 111133,
   HD 118022, and HD 164258 we present here more refined values of the period.
   No variability has been detected for the star HD 137949 within a time scale
   of the order of ten days.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table">
	<title>Observations</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Star1</name>
			<definition>Star name</definition>
			<units>---</units></field>
		<field>
			<name>Star2</name>
			<definition>References star</definition>
			<units>---</units></field>
		<field>
			<name>HJD</name>
			<definition>Heliocentric julian day</definition>
			<units>d</units></field>
		<field>
			<name>n_HJD</name>
			<definition>Data marked with an asterisk are not
                                   reported on Fig. 3</definition>
			<units>---</units></field>
		<field>
			<name>Du</name>
			<definition>Magnitude difference (star1-star2) in u</definition>
			<units>mag</units></field>
		<field>
			<name>Dv</name>
			<definition>Magnitude difference (star1-star2) in v</definition>
			<units>mag</units></field>
		<field>
			<name>Db</name>
			<definition>Magnitude difference (star1-star2) in b</definition>
			<units>mag</units></field>
		<field>
			<name>Dy</name>
			<definition>Magnitude difference (star1-star2) in y</definition>
			<units>mag</units></field></fields></tableHead>
	
			<textFile xlink:href="table.tex"><name>table.tex</name><description><para>LaTeX version of table</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Sep</month><day>01</day></date></ingest>
		</history>
	<identifier>J_A+AS_108_595.xml</identifier></dataset>
