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J/AJ/115/168        Kinematics of red giant and RR Lyrae stars (Chiba+ 1998)
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Early evolution of the Galactic halo revealed from Hipparcos observations of
metal-poor stars
       Chiba M., Yoshii Y.
      <Astron. J. 115, 168 (1998)>
      =1998AJ....115..168C      (SIMBAD/NED BibCode)
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ADC_Keywords: Stars, giant ; Stars, variable ; Proper motions
Mission_Name: Hipparcos
Keywords: Galaxy: abundances - Galaxy: evolution - Galaxy: halo

Abstract:
    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]<=-1 and thus represent the old stellar populations in the
    Galaxy. The halo component, with [Fe/H]<=-1.6, is characterized by a
    lack of systemic rotation
    [(<U>, <V>, <W>)=(16+/-18, -217+/-21, -10+/-12)km/s] and a radially
    elongated velocity ellipsoid
    [(<U>, <V>, <W>)=(161+/-10, 115+/-7, 108+/-7)km/s]. About 16% of such
    metal-poor stars have low orbital eccentricities (e<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]<=-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<[Fe/H]<=-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|<1kpc. This disk
    component appears to constitute only 10% for -1.6<[Fe/H]<=-1 and 20%
    for -1.4<[Fe/H]<=-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.

File Summary:
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  FileName      Lrecl  Records   Explanations
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ReadMe             80        .   This file
table1.dat        127      298   Program stars
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See also:
    I/196 : Hipparcos Input Catalogue, Version 2 (Turon+ 1993)
    I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)

Byte-by-byte Description of file: table1.dat
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   Bytes Format  Units       Label     Explanations
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   1-  2  A2     ---         Type      [RG] Type of the stars
                                             RG: Red giants; RR: RR Lyrae
   4-  9  I6     ---         HIC(P)    HIC or HIP (Cat. <I/239>) number
  11- 22  A12    ---         Name      Other name
  24- 29  F6.2   mas         plx       Trigonometric parallax
  31- 35  F5.2   mas       e_plx       rms uncertainty on plx
  37- 43  F7.2   mas/yr      pmRA*     Proper motion in RA time cos{delta}
  45- 49  F5.2   mas/yr    e_pmRA*     rms uncertainty on pmRA
  51- 57  F7.2   mas/yr      pmDE      Proper motion in DE
  59- 63  F5.2   mas/yr    e_pmDE      rms uncertainty on pmDE
  65- 69  F5.3   kpc         Dist      ? Photometric distance
  71- 75  F5.3   kpc       e_Dist      ? rms uncertainty on Dist
  77- 81  F5.2  [Sun]        [Fe/H]    ? Metallicity
  83- 86  F4.2  [Sun]      e_[Fe/H]    ? rms uncertainty on [Fe/H]
  88- 94  F7.2   km/s        RV        ? Radial velocity
  96-100  F5.2   km/s      e_RV        ? rms uncertainty on RV
 102-107  F6.3   arcsec/yr   pmRAold   ? Old proper motion in RA
 109-114  F6.3   arcsec/yr   pmDEold   ? Old proper motion in DE
 116-117  A2     ---       r_Dist      References for Dist and [Fe/H] (1)
     118  A1     ---         ---       [/]
 119-123  A5     ---       r_RV        References for RV (2)
     124  A1    ---          ---       [/]
     125  I1    ---        r_pmRA*     ? References for proper motions (3)
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Note (1): 1: Anthony-Twarog & Twarog, 1994AJ....107.1577A, Cat. <J/AJ/107/1577>
         1s: Spectroscopic abundances compiled by Anthony-Twarog & Twarog, 1994
          2: Bond, 1980ApJS...44..517B
         2s: Spectroscopic abundances compiled by Anthony-Twarog & Twarog, 1994
          3: Layden, 1994AJ....108.1016L, Cat. <J/AJ/108/1016>
          4: Layden et al., 1996AJ....112.2110L
Note (2): 1: Bond 1980ApJS...44..517B
          2: Carney & Latham, 1986AJ.....92...60C
          3: Norris, Bessell & Pickles, 1985
          4: Barbier-Brossat, 1989A&AS...80...67B, Cat. <III/161>
          5: Wilson, 1953, Cat. <III/21>
          6: Evans, 1978BICDS..15..121J, Cat. <III/42>
          7: Griffin et al., 1982MNRAS.198..637G
          8: Papers quoted by Bond, 1980ApJS...44..517B
          9: Layden, 1994AJ....108.1016L, Cat. <J/AJ/108/1016>
Note (3): 1: Lick Northern Proper Motion Catalogue, Cat. <I/199>
          2: Hipparcos Input Catalogue, Cat. <I/196>
          3: Wan, Mao & Ji, 1980, Ann. Shanghai Obs., 2, 1
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History: Copied from the electronic version of AJ
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(End)                                          Patricia Bauer [CDS]  10-Mar-1998

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