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J/ApJ/496/39        Properties of poor groups of galaxies. I. (Zabludoff+ 1998)
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The properties of poor groups of galaxies. I. Spectroscopic survey and results.
       Zabludoff A.I., Mulchaey J.S.
      <Astrophys. J. 496, 39 (1998)>
      =1998ApJ...496...39Z      (SIMBAD/NED BibCode)
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ADC_Keywords: Clusters, galaxy ; Radial velocities
Keywords: galaxies: clusters: general - galaxies: distances and redshifts -
          galaxies: elliptical and lenticular, cD - galaxies: evolution -
          galaxies: interaction - large-scale structure of universe -
          X-rays: galaxies

Abstract:
    We use multifiber spectroscopy of 12 poor groups of galaxies to
    address (1) whether the groups are bound systems or chance projections
    of galaxies along the line of sight; (2) why the members of each group
    have not already merged to form a single galaxy, despite the groups'
    high galaxy densities, short crossing times, and likely environments
    for galaxy-galaxy mergers; and (3) how galaxies might evolve in these
    groups, where the collisional effects of the intragroup gas and the
    tidal influences of the global potential are weaker than in rich
    clusters. Each of the 12 groups has fewer than about five cataloged
    members in the literature. Our sample consists of 1002 galaxy
    velocities, 280 of which are group members. The groups have mean
    recessional velocities between 1600 and 7600km/s. Nine groups,
    including three Hickson compact groups, have the extended X-ray
    emission characteristic of an intragroup medium (see Paper II,
    1998ApJ...496...73M).

File Summary:
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  FileName        Lrecl  Records   Explanations
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ReadMe             80        .   This file
table1.dat         50     1002   Galaxy data
table2.dat         81       12   Group kinematic properties
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Byte-by-byte Description of file: table1.dat
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   Bytes Format Units   Label    Explanations
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   1- 10  A10   ---     Name     Galaxy name
  13- 14  I2    h       RAh      Right ascension (J2000.0)
  16- 17  I2    min     RAm      Right ascension (J2000.0)
  19- 22  F4.1  s       RAs      Right ascension (J2000.0)
      24  A1    ---     DE-      Declination sign
  25- 26  I2    deg     DEd      Declination (J2000.0)
  28- 29  I2    arcmin  DEm      Declination (J2000.0)
  31- 32  I2    arcsec  DEs      Declination (J2000.0)
  34- 38  I5    km/s    HRV      Heliocentric radial velocity (1)
  40- 42  I3    km/s  e_HRV      rms uncertainty on HRV
      44  I1    ---     Line     [0/2] Type of measurement (2)
      46  A1    ---     MType    [ES] Morphological type (3)
      48  A1    ---     Plate    [pc] Plate/CCD (4)
      50  A1    ---   r_HRV      [N0] Heliocentric radial velocity reference (5)
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Note (1): The velocities are either emission-line velocities, absorption-line
           velocities, or a weighted average of the two
Note (2): 0: absorption lines
          1: emission lines
          2: combination of both
Note (3): E: early type
          S: late type
Note (4): p: plate
          c: CCD
Note (5): N: from NED
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Byte-by-byte Description of file: table2.dat
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   Bytes Format Units     Label   Explanations
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   1-  8  A8    ---       Group   Group name
  10- 11  I2    h         RAh     Right ascension of the group optical
                                   projected centroid in J2000
  13- 14  I2    min       RAm     Right ascension of the group optical
                                   projected centroid in J2000
  16- 19  F4.1  s         RAs     Right ascension of the group optical
                                   projected centroid in J2000
      21  A1    ---       DE-     Declination sign
  22- 23  I2    deg       DEd     Declination of the group optical
                                   projected centroid in J2000
  25- 26  I2    arcmin    DEm     Declination of the group optical
                                   projected centroid in J2000
  28- 29  I2    arcsec    DEs     Declination of the group optical
                                   projected centroid in J2000
  31- 33  I3    ---       Ntot    Total number of galaxies with measured
                                   redshifts in the fiber field
  35- 36  I2    ---       Ngroup  Number of group members
  38- 41  I4    km/s      HRV     Biweight estimators of the mean
                                   heliocentric velocity
  43- 44  I2    km/s    e_HRV     rms uncertainty on HRV
  46- 48  I3    km/s      sigma   Line-of-sight velocity dispersion
  50- 52  I3    km/s    E_sigma   Error on sigma (upper limit)
  54- 55  I2    km/s    e_sigma   Error on sigma (lower limit)
  57- 60  F4.2  Mpc       rsample Physical radius of the group sampled by the
                                  fiber field (h^-1^Mpc)
  62- 65  F4.2  Mpc       rp      ? Pair radius (h^-1^Mpc)
  67- 70  F4.2  Mpc       rh      ? Mean harmonic (virial )radius (h^-1^Mpc)
  72- 76  E5.1  solMass   Mvir    ? Virial mass (h^-1^Mpc)
  78- 81  F4.2  ---       tc/tH   ? Ratio of the crossing time to Hubble time
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History: From ApJ electronic version
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(End)                           James Marcout, Patricia Bauer [CDS]  15-Jun-1998

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