<?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>Deep HST V- and I-band observations of two globular clusters in the halo of M31</title>
	<altname type="ADC">J/AJ/114/1488</altname>
		<altname type="CDS">J/AJ/114/1488</altname>
		<altname type="brief">Globulars in M31</altname>
	<reference>
		<source>
<journal>
	<title>Deep HST V- and I-band observations of two globular clusters in the halo of M31</title>
	<author>
			<initial>S</initial>
			<lastName>Holland</lastName></author>
	<author>
			<initial>G</initial>
			<initial>G</initial>
			<lastName>Fahlman</lastName></author>
	<author>
			<initial>H</initial>
			<initial>B</initial>
			<lastName>Richer</lastName></author>
	<name>Astron. J.</name>
	<volume>114</volume>
	<pageno>1488</pageno>
		<date>
			<year>1997</year></date>
	<bibcode>1997AJ....114.1488H</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.html">Photometry</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    We present deep (V=~27) V- and I-band stellar photometry of G302 and
    G312, two globular star clusters in the halo of M31. These data were
    obtained using the Hubble Space Telescope's Wide Field/Planetary
    Camera 2. We find iron abundances of [Fe/H]=-1.85+/-0.12 for G302
    and [Fe/H]=-0.56+/-0.03 for G312, consistent with spectroscopic
    measurements. The color-magnitude diagrams for each cluster show no
    evidence for an intermediate-aged population of stars, or a second
    parameter effect in the morphology of the horizontal branch. G302
    shows no evidence for a color gradient but the inner regions of G312
    are bluer than the outer regions. G312 shows no evidence of
    ellipticity or an extended halo of stars. G302 has a projected
    ellipticity of {epsilon}=0.195+/-0.012 with the projected major axis
    oriented towards the center of M31. G302 also shows evidence of an
    extended asymmetric stellar halo extending to at least twice the
    fitted Michie-King tidal radius. The amount of mass beyond the tidal
    radius of G302 is consistent with the stellar escape rates which have
    been predicted by N-body simulations of globular clusters in the
    Galactic tidal field.
    (c) 1997 American Astronomical Society.</para></abstract>
                        <details><para><observatory base="space"> HST</observatory></para>
	<astroObjects>
		
			<astroObject><name>G302</name><name>SKHB 302</name><name>Bol 240</name><position><ra>00 45 25.2</ra><dec>+41 05 30</dec></position></astroObject>
			<astroObject><name>G312</name><name>SKHB 312</name><name>Bol 379</name><position><ra>00 45 58.8</ra><dec>+40 42 32</dec></position></astroObject></astroObjects></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table3.dat">
	<title>Stellar photometry for G302 and the surrounding fields</title></tableLink>
				<tableLink xlink:href="table4.dat">
	<title>Stellar photometry for G312 and the surrounding fields</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>CCD</name>
			<definition>CCD the star was observed on</definition>
			<units>---</units></field>
		<field>
			<name>ID</name>
			<definition>Identification number
	<footnote footnoteId="???"><para>number=1</para>
			<para>Identification numbers are only unique for stars on a given CCD.</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>Xpos</name>
			<definition>X pixel coordinate
	<footnote footnoteId="???"><para>number=2</para>
			<para>1 pix = 0.1".
</para></footnote></definition>
			<units>pix</units></field>
		<field>
			<name>Ypos</name>
			<definition>Y pixel coordinate
	<footnote footnoteId="???"><para>number=2</para>
			<para>1 pix = 0.1".
</para></footnote></definition>
			<units>pix</units></field>
		<field>
			<name>Vmag</name>
			<definition>V-band magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Vmag</name>
			<definition>1-sigma uncertainty in Vmag</definition>
			<units>mag</units></field>
		<field>
			<name>2_Vmag</name>
			<definition>Value of the DAOPHOT Chi statistics for Vmag</definition>
			<units>---</units></field>
		<field>
			<name>Imag</name>
			<definition>I-band magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Imag</name>
			<definition>1-sigma uncertainty in Imag</definition>
			<units>mag</units></field>
		<field>
			<name>2_Imag</name>
			<definition>Value of the DAOPHOT Chi statistics for Imag</definition>
			<units>---</units></field></fields></tableHead>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table5.dat">
	<title>Stellar photometry for G302</title></tableLink>
				<tableLink xlink:href="table6.dat">
	<title>Stellar Photometry for G312</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>CCD</name>
			<definition>CCD the star was observed on</definition>
			<units>---</units></field>
		<field>
			<name>ID</name>
			<definition>Identification number</definition>
			<units>---</units></field>
		<field>
			<name>Xpos</name>
			<definition>X pixel coordinate
	<footnote footnoteId="???"><para>number=1</para>
			<para>1 pix = 0.1".
</para></footnote></definition>
			<units>pix</units></field>
		<field>
			<name>Ypos</name>
			<definition>Y pixel coordinate
	<footnote footnoteId="???"><para>number=1</para>
			<para>1 pix = 0.1".
</para></footnote></definition>
			<units>pix</units></field>
		<field>
			<name>Dist</name>
			<definition>Distance of star from cluster center</definition>
			<units>arcsec</units></field>
		<field>
			<name>Vmag</name>
			<definition>V-band magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Vmag</name>
			<definition>1-sigma uncertainty in Vmag</definition>
			<units>mag</units></field>
		<field>
			<name>2_Vmag</name>
			<definition>Value of the DAOPHOT Chi statistics for Vmag</definition>
			<units>---</units></field>
		<field>
			<name>Imag</name>
			<definition>I-band magnitude</definition>
			<units>mag</units></field>
		<field>
			<name>e_Imag</name>
			<definition>1-sigma uncertainty in Imag</definition>
			<units>mag</units></field>
		<field>
			<name>2_Imag</name>
			<definition>Value of the DAOPHOT Chi statistics for Imag</definition>
			<units>---</units></field></fields></tableHead>
	
			<textFile xlink:href="tables.tex"><name>tables.tex</name><description><para>AASTeX version of the tables</para></description></textFile>
			<textFile xlink:href="tables.ps" type="postscript"><name>tables.ps</name><description><para>PostScript version of the tables</para></description></textFile>
	<history>
		<ingest>
	
			<creator>
				<staff/>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1998</year><month>Feb</month><day>05</day></date><acknowledgement>AAS CD-ROM series, Volume 9, 1997         Lee Brotzman [ADS] 04-Nov-1997</acknowledgement></ingest>
		</history>
	<identifier>J_AJ_114_1488.xml</identifier></dataset>
