<?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>Early evolution of the Galactic halo revealed from Hipparcos observations of
metal-poor stars</title>
	<altname type="ADC">J/AJ/115/168</altname>
		<altname type="CDS">J/AJ/115/168</altname>
		<altname type="brief">Kinematics of red giant and RR Lyrae stars</altname>
	<reference>
		<source>
<journal>
	<title>Early evolution of the Galactic halo revealed from Hipparcos observations of
metal-poor stars</title>
	<author>
			<initial>M</initial>
			<lastName>Chiba</lastName></author>
	<author>
			<initial>Y</initial>
			<lastName>Yoshii</lastName></author>
	<name>Astron. J.</name>
	<volume>115</volume>
	<pageno>168</pageno>
		<date>
			<year>1998</year></date>
	<bibcode>1998AJ....115..168C</bibcode></journal></source>
	<related>
			<holding role="similar">I/196 : Hipparcos Input Catalogue, Version 2 (Turon+ 1993)<xlink:simple href="I/196"/></holding>
			<holding role="similar">I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)<xlink:simple href="I/239"/></holding></related></reference>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/adc_keywords.html">
			<keyword xlink:href="Proper_motions.html">Proper motions</keyword>
			<keyword xlink:href="Stars_giant.html">Stars, giant</keyword>
			<keyword xlink:href="Stars_variable.html">Stars, variable</keyword></keywords>
	<keywords parentListURL="http://messier.gsfc.nasa.gov/xml/keywordlists/apj_keywords.html">
			<keyword xlink:href="Galaxy_abundances.html">Galaxy: abundances</keyword>
			<keyword xlink:href="Galaxy_evolution.html">Galaxy: evolution</keyword>
			<keyword xlink:href="Galaxy_halo.html">Galaxy: halo</keyword></keywords>
	<descriptions>
				<abstract>
					<para>
    The kinematics of 122 red giant and 124 RR Lyrae stars in the solar
    neighborhood are studied using accurate measurements of their proper
    motions obtained by the Hipparcos astrometry satellite, combined with
    their published photometric distances, metal abundances, and radial
    velocities. A majority of these sample stars have metal abundances of
    [Fe/H]&lt;=-1 and thus represent the old stellar populations in the
    Galaxy. The halo component, with [Fe/H]&lt;=-1.6, is characterized by a
    lack of systemic rotation
    [(&lt;U>, &lt;V>, &lt;W>)=(16+/-18, -217+/-21, -10+/-12)km/s] and a radially
    elongated velocity ellipsoid
    [(&lt;U>, &lt;V>, &lt;W>)=(161+/-10, 115+/-7, 108+/-7)km/s]. About 16% of such
    metal-poor stars have low orbital eccentricities (e&lt;0.4), and we see
    no evidence of a correlation between [Fe/H] and e. Based on the model
    for the e-distribution of orbits, we show that this fraction of low-e
    stars for [Fe/H]&lt;=-1.6 is explained by the halo component alone,
    without introducing the extra disk component claimed by recent
    workers. This is also supported by the absence of a significant change
    in the e-distribution with height from the Galactic plane. In the
    intermediate-metallicity range (-1.6&lt;[Fe/H]&lt;=-1), we find that stars
    with disklike kinematics have only modest effects on the distributions
    of rotational velocities and e for the sample at |z|&lt;1kpc. This disk
    component appears to constitute only 10% for -1.6&lt;[Fe/H]&lt;=-1 and 20%
    for -1.4&lt;[Fe/H]&lt;=-1. It is also verified that this metal-weak disk has
    a mean rotation of ~195km/s and a vertical extent of 1 kpc, which is
    consistent with the thick disk's dominating at [Fe/H]=-0.6 to -1. We
    find no metallicity gradient in the halo, whereas there is an
    indication of a metallicity gradient in the metal-weak tail of the
    thick disk. The implications of these results for the early evolution
    of the Galaxy are also presented.</para></abstract>
                        <details><para><observatory base="space"> Hipparcos</observatory></para></details></descriptions>
	<tableHead>
		<tableLinks>
				<tableLink xlink:href="table1.dat">
	<title>Program stars</title></tableLink></tableLinks>
	<fields>
		<field>
			<name>Type</name>
			<definition>Type of the stars
                                             RG: Red giants; RR: RR Lyrae</definition>
			<units>---</units></field>
		<field>
			<name>HIC(P)</name>
			<definition>HIC or HIP (Cat. &lt;I/239>) number</definition>
			<units>---</units></field>
		<field>
			<name>Name</name>
			<definition>Other name</definition>
			<units>---</units></field>
		<field>
			<name>plx</name>
			<definition>Trigonometric parallax</definition>
			<units>mas</units></field>
		<field>
			<name>e_plx</name>
			<definition>rms uncertainty on plx</definition>
			<units>mas</units></field>
		<field>
			<name>pmRA*</name>
			<definition>Proper motion in RA time cos{delta}</definition>
			<units>mas/yr</units></field>
		<field>
			<name>e_pmRA*</name>
			<definition>rms uncertainty on pmRA</definition>
			<units>mas/yr</units></field>
		<field>
			<name>pmDE</name>
			<definition>Proper motion in DE</definition>
			<units>mas/yr</units></field>
		<field>
			<name>e_pmDE</name>
			<definition>rms uncertainty on pmDE</definition>
			<units>mas/yr</units></field>
		<field>
			<name>Dist</name>
			<definition>Photometric distance</definition>
			<units>kpc</units></field>
		<field>
			<name>e_Dist</name>
			<definition>rms uncertainty on Dist</definition>
			<units>kpc</units></field>
		<field>
			<name>[Fe/H]</name>
			<definition>Metallicity</definition>
			<units>[Sun]</units></field>
		<field>
			<name>e_[Fe/H]</name>
			<definition>rms uncertainty on [Fe/H]</definition>
			<units>[Sun]</units></field>
		<field>
			<name>RV</name>
			<definition>Radial velocity</definition>
			<units>km/s</units></field>
		<field>
			<name>e_RV</name>
			<definition>rms uncertainty on RV</definition>
			<units>km/s</units></field>
		<field>
			<name>pmRAold</name>
			<definition>Old proper motion in RA</definition>
			<units>arcsec/yr</units></field>
		<field>
			<name>pmDEold</name>
			<definition>Old proper motion in DE</definition>
			<units>arcsec/yr</units></field>
		<field>
			<name>r_Dist</name>
			<definition>References for Dist and [Fe/H]
	<footnote footnoteId="???"><para>number=1</para>
			<para>1: Anthony-Twarog &amp; Twarog, 1994AJ....107.1577A, Cat. &lt;J/AJ/107/1577>
         1s: Spectroscopic abundances compiled by Anthony-Twarog &amp; Twarog, 1994
          2: Bond, 1980ApJS...44..517B
         2s: Spectroscopic abundances compiled by Anthony-Twarog &amp; Twarog, 1994
          3: Layden, 1994AJ....108.1016L, Cat. &lt;J/AJ/108/1016>
          4: Layden et al., 1996AJ....112.2110L</para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>---</name>
			<definition/>
			<units>---</units></field>
		<field>
			<name>r_RV</name>
			<definition>References for RV
	<footnote footnoteId="???"><para>number=2</para>
			<para>1: Bond 1980ApJS...44..517B
          2: Carney &amp; Latham, 1986AJ.....92...60C
          3: Norris, Bessell &amp; Pickles, 1985
          4: Barbier-Brossat, 1989A&amp;AS...80...67B, Cat. &lt;III/161>
          5: Wilson, 1953, Cat. &lt;III/21>
          6: Evans, 1978BICDS..15..121J, Cat. &lt;III/42>
          7: Griffin et al., 1982MNRAS.198..637G
          8: Papers quoted by Bond, 1980ApJS...44..517B
          9: Layden, 1994AJ....108.1016L, Cat. &lt;J/AJ/108/1016></para></footnote></definition>
			<units>---</units></field>
		<field>
			<name>---</name>
			<definition/>
			<units>---</units></field>
		<field>
			<name>r_pmRA*</name>
			<definition>References for proper motions
	<footnote footnoteId="???"><para>number=3</para>
			<para>1: Lick Northern Proper Motion Catalogue, Cat. &lt;I/199>
          2: Hipparcos Input Catalogue, Cat. &lt;I/196>
          3: Wan, Mao &amp; Ji, 1980, Ann. Shanghai Obs., 2, 1
</para></footnote></definition>
			<units>---</units></field></fields></tableHead>
	
	<history>
		<ingest>
	
			<creator>
				<lastName>Patricia Bauer</lastName>
				<affiliation>CDS</affiliation></creator>
	<date>
		<year>1998</year><month>Mar</month><day>10</day></date></ingest>
		
		<revisions>
	<revision>
		<creator>
			<lastName>UNKNOWN</lastName></creator>
		<date><year>UNKNOWN</year></date>
		<para> Copied from the electronic version of AJ</para></revision></revisions></history>
	<identifier>J_AJ_115_168.xml</identifier></dataset>
