<?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 young Magellanic cluster NGC 2004</title>
	<altname type="ADC">J/AJ/102/137</altname>
		<altname type="CDS">J/AJ/102/137</altname>
		<altname type="brief">NGC 2004</altname>
	<reference>
		<source>
<journal>
	<title>The young Magellanic cluster NGC 2004</title>
	<author>
			<initial>D</initial>
			<lastName>Bencivenni</lastName></author>
	<author>
			<initial>E</initial>
			<lastName>Brocato</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Buonanno</lastName></author>
	<author>
			<initial>V</initial>
			<lastName>Castellani</lastName></author>
	<name>Astron. J.</name>
	<volume>102</volume>
	<pageno>137</pageno>
		<date>
			<year>1991</year></date>
	<bibcode>1991AJ....102..137B</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_galaxy.html">Clusters, galaxy</keyword>
			<keyword xlink:href="Galaxies_nearby.html">Galaxies, nearby</keyword>
			<keyword xlink:href="Photometry_BV.html">Photometry, BV</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
   The results of a new CCD photometric investigation of stars in the field
   of the LMC cluster NGC 2004 are reported and discussed. B, V photometry
   is given for more than 1500 objects, the large majority to be ascribed
   to the cluster. A new color-magnitude diagram is presented. It shows a
   well-defined blue sequence (BS) of H-burning stars, running from
   V~=21mag up to V~=13mag, together with a group of cluster He-burning red
   supergiants with V~=13mag and a clump of field red giants at about
   V~=19 mag. Theoretical evolutionary computations are reported covering
   the range of massive stars evolving in the cluster. These evolutionary
   tracks can match the observed CM diagram provided that a low efficiency
   of the surface convection (a low value of the mixing length) is adopted.
   Comparison of the theoretical luminosity function with the upper portion
   of the observed BS distribution suggests a cluster age of about
   8 million years, in agreement with previous evaluations. The completeness
   of the sample and the contribution of field stars have been estimated.
   The CM distribution of cluster stars has been compared with the results
   of synthetic clusters based on the adopted evolutionary scenario. We find
   that the observed distribution of cluster stars in the different
   evolutionary phases appears in good agreement with prediction
   based on theoretical evolutionary lifetimes. Moreover, the distribution
   of H-burning stars agrees with a Salpeter distribution in the whole
   range 2&lt;=M/M_{sun}_&lt;=20. After a short review of the current theoretical
   scenario concerning massive stars, the CM diagram of field stars is
   discussed, reaching the conclusion that the observed clump of red giants
   is the natural consequence of the peculiar large lifetimes in the central
   He burning phase of stars with M~=3M_{sun}_.</para></abstract>
                        <details/></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table2">
	<title>Program stars magnitudes, colors and positions</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>No</name>
			<definition>Star identification number</definition>
			<units>---</units></field>
		<field>
			<name>Vmag</name>
			<definition>V magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>B-V</name>
			<definition>B-V colour</definition>
			<units>mag</units></field>
		<field>
			<name>X</name>
			<definition>X position</definition>
			<units>pix</units></field>
		<field>
			<name>Y</name>
			<definition>Y position</definition>
			<units>pix</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1994</year><month>Dec</month><day>09</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Keypunched at CDS</para></revision></revisions></history>
	<identifier>J_AJ_102_137.xml</identifier></dataset>
