<?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>Globular clusters 1 and 3 in the Fornax dwarf galaxy</title>
	<altname type="ADC">J/A+A/317/54</altname>
		<altname type="CDS">J/A+A/317/54</altname>
		<altname type="brief">Fornax cluster 1 and 3 photometry</altname>
	<reference>
		<source>
<journal>
	<title>Globular clusters 1 and 3 in the Fornax dwarf galaxy</title>
	<author>
			<initial>U</initial>
			<initial>G</initial>
			<lastName>Jorgensen</lastName></author>
	<author>
			<initial>R</initial>
			<lastName>Jimemez</lastName></author>
	<name>Astron. Astrophys.</name>
	<volume>317</volume>
	<pageno>54</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997A&amp;A...317...54J</bibcode></journal></source></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Clusters_globular.html">Clusters, globular</keyword>
			<keyword xlink:href="Photometry_CCD.html">Photometry, CCD</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="galaxies_formation.html">galaxies: formation</keyword>
			<keyword xlink:href="galaxies_individual_(Fornax_dSph_A0237-34).html">galaxies: individual (Fornax dSph, A0237-34)</keyword>
			<keyword xlink:href="galaxies_star_clusters.html">galaxies: star clusters</keyword>
			<keyword xlink:href="stars_AGB_and_post-AGB.html">stars: AGB and post-AGB</keyword>
			<keyword xlink:href="stars_carbon.html">stars: carbon</keyword></keywords>
	<descriptions>
				<description>
				<para>
    We have performed photometric CCD observations of the giant and
    horizontal branches of the globular cluster1, and of the giant branch
    of cluster3, in the Fornax dwarf spheroidal galaxy. The observations
    were performed in the V and I standard broad-band filters as well as
    through two narrow-band filters especially designed to distinguish
    between carbon and M type stars. The AGB is richly populated with
    carbon-rich stars, and all of them are considerably below the
    theoretical lower luminosity limit for such stars. If the Fornax
    clusters are interpreted as resembling an earlier epoch of the
    Galactic globular clusters, the low luminosities of the carbon stars
    therefore point to a larger role of the low-mass stars in the chemical
    enrichment of our Galaxy. The giant branches of the Fornax clusters
    are much broader than canonical giant branches in Galactic globulars,
    and the AGB is more well populated. We suggest that the morphology and
    stellar population of the giant branches indicate that the dwarf
    galaxies are =~3Gyr younger than the Galactic halo, which in turn
    seems to be =~3Gyr younger than the Galactic globular clusters.
    For a description of the N2-N3 photometric system, see e.g. &lt;GCPD/39></para></description>
                        <details>
	<astroObjects>
		
			<astroObject><name>Cluster 1 in Fornax</name><position><ra>02 37.0 </ra><dec>-34 11 </dec></position></astroObject>
			<astroObject><name>Cluster 3 in Fornax</name><position><ra>02 39.8 </ra><dec>-34 16 </dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1">
	<title>Cluster 1 photometry</title></tableLink>
				<tableLink xlink:href="table2">
	<title>Cluster 3 photometry</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>ID</name>
			<definition>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 color index</definition>
			<units>mag</units></field>
		<field>
			<name>logL</name>
			<definition>Reduced luminosity</definition>
			<units>solLum</units></field>
		<field>
			<name>logTeff</name>
			<definition>Effective temperature</definition>
			<units>K</units></field>
		<field>
			<name>Mbol</name>
			<definition>Absolute bolometric magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>81-78</name>
			<definition>Narrow band color
                                     {DELTA}m_(81-78)_=m(8120A)-m(7795A)</definition>
			<units>mag</units></field>
		<field>
			<name>N2</name>
			<definition>Number in Buonanno et al. (1985) catalogue</definition>
			<units>---</units></field>
		<field>
			<name>Vmag2</name>
			<definition>V magnitude in Buonanno et al. (1985)</definition>
			<units>mag</units></field>
		<field>
			<name>N3</name>
			<definition>Number in Demers et al. (1990) catalogue
	<footnote footnoteId="???"><para>number=1</para>
			<para>These data are only in table1
</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Vmag3</name>
			<definition>V magnitude in Demers et al. (1990)
	<footnote footnoteId="???"><para>number=1</para>
			<para>These data are only in table1
</para></footnote></definition>
			<units>mag</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>Jun</month><day>03</day></date><acknowledgement>Raul Jimenez &lt;R.Jimenez@roe.ac.uk></acknowledgement></ingest>
		</history>
	<identifier>J_A+A_317_54.xml</identifier></dataset>
