Astronomical Data Center

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/journal_tables/MNRAS/326/473/

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J/MNRAS/326/473  Vel. Distribution of low-luminosity E galaxies (Halliday+ 2001)
================================================================================
Line-of-sight velocity distributions of low-luminosity elliptical galaxies
    Halliday C., Davies R. L., Kuntschner H., Birkinshaw M., Bender R.,
    Saglia R.P., Baggley G.
   <Mon. Not. R. Astron. Soc., 326, 473 (2001)>
   =2001MNRAS.326..473H
================================================================================
ADC_Keywords: Galaxies, rotation ; Velocity dispersion
Keywords: galaxies: formation ; galaxies: elliptical and lenticular ;
          galaxies: kinematics and dynamics

Description:
    The shape of the line-of-sight velocity distribution (LOSVD) is
    measured for a sample of 14 elliptical galaxies, predominantly
    low-luminosity ellipticals. The sample is dominated by galaxies in the
    Virgo cluster but also contains ellipticals in nearby groups and low
    density environments. The parameterization of the LOSVD due to Gerhard
    and van der Marel & Franx is adopted, which measures the asymmetrical
    and symmetrical deviations of the LOSVD from a Gaussian by the
    amplitudes h3 and h4 of the Gauss-Hermite series. Rotation, velocity
    dispersion, h3 and h4 are determined as a function of radius for both
    major and minor axes using the Fourier Correlation Quotient method of
    Bender (1990). Galaxy spectra are rebinned in the direction of the
    spectroscopic slit to a minimum signal-to-noise ratio (S/N) of 60 per
    angstrom. Rotation and velocity dispersion are determined separately
    for S/N = 30 per angstrom.

File Summary:
--------------------------------------------------------------------------------
 FileName    Lrecl    Records    Explanations
--------------------------------------------------------------------------------
ReadMe          80         .     This file
galaxies.dat    82        14     Description of galaxy sample
kinem1.dat      76       427     Line-of-sight Velocity Distribution (LOSVD)
                                  measurements for S/N = 60 per angstrom
kinem2.dat      52       787     Rotation and velocity dispersion for
                                 S/N = 30 per angstrom
--------------------------------------------------------------------------------

See also:
  VII/155 : Third Reference Cat. of Bright Galaxies (RC3) (de Vaucouleurs+ 1991)

Byte-by-byte Description of file: galaxies.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  2  I2    h        RAh      Right Ascension J2000 (hours)
   4-  5  I2    min      RAm      Right Ascension J2000 (minutes)
   7- 10  F4.1  s        RAs      Right Ascension J2000 (seconds)
      12  A1    ---      DE-      Declination J2000 (sign)
  13- 14  I2    deg      DEd      Declination J2000 (degrees)
  16- 17  I2    arcmin   DEm      Declination J2000 (minutes)
  19- 20  I2    arcsec   DEs      Declination J2000 (seconds)
  22- 29  A8     ---     Name     Name of galaxy
  33- 35  A3     ---     Type     Galaxy Hubble type (1)
  37- 41  F5.2   mag     BT       Photoelectric total apparent magnitude (1)
  44- 48  F5.2   arcsec  Re       Effective radius (1)
  51- 54  F4.2   ---     epsilon  Ellipticity (2)
  57- 60  I4     km/s    czhelio  Heliocentric redshift (1)
  63- 67  F5.1   mag     MB       Total absolute magnitude (3)
  71- 82  A12    ---     environ  Environment of galaxy (4)
--------------------------------------------------------------------------------
Note (1): All taken from the Third Reference Catalogue (RC3) 
     (de Vaucouleurs et al. 1991, Cat. <VII/155>);
     Hubble types are: E-elliptical, S-spiral, S0-lenticular,
     +-intermediate (i.e. between elliptical and S0),
     ?-doubtful classification.

Note (2): Values taken from Peletier et al. (1990, Cat. <J/AJ/100/109>),
    Bender et al. (1989A&A...217...35B) and Lauer et al.
    (1995AJ....110.2622L); for NGC's 4339, 4458, 4468, 5582 values are
    obtained using the Digital Sky Survey.

Note (3): Calculated using distances based on the 
    surface-brightness-fluctuation survey of Tonry et al. (2001ApJ...546..681T).

Note (4): Indicates whether each galaxy is a member of the Virgo cluster, 
    the Leo I group, the Leo II group or resides in a low density
    environment (-).
--------------------------------------------------------------------------------

Byte-by-byte Description of file: kinem1.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  8  A8     ---     Name     Name of galaxy
   9- 10  A2     ---   n_Name     [MJN] Major or Minor axis (1)
  13- 18  F6.2   arcsec  Rad      [-41/46] Radius from galaxy centre
  21- 26  F6.1   km/s    Vrot     Rotation velocity
  28- 32  F5.1   km/s  e_Vrot     Error in rotation velocity
  35- 39  F5.1   km/s    sigma    Velocity dispersion
  42- 46  F5.1   km/s  e_sigma    Error in velocity dispersion
  49- 54  F6.3   ---     h4       Gauss-Hermite coefficient h4
  56- 61  F6.3   ---   e_h4       Error in Gauss-Hermite coefficient h4
  63- 68  F6.3   ---     h3       Gauss-Hermite coefficient h3
  70- 75  F6.3   ---   e_h3       Error in Gauss-Hermite coefficient h3
--------------------------------------------------------------------------------
Note (1): Indication of axis of galaxy studied:
     MJ = major axis and MN = minor axis
--------------------------------------------------------------------------------

Byte-by-byte Description of file: kinem2.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   1-  8  A8     ---     Name     Name of galaxy
   9- 10  A2     ---   n_Name     [MJN] Major or Minor axis (1)
  13- 18  F6.2   arcsec  Rad      [-54/54] major axis radius from galaxy centre
  21- 26  F6.1   km/s    Vrot     major axis rotation velocity
  28- 33  F6.1   km/s  e_Vrot     major axis error in rotation velocity
  36- 40  F5.1   km/s    sigma    major axis velocity dispersion
  42- 46  F5.1   km/s  e_sigma    major axis error in velocity dispersion
--------------------------------------------------------------------------------
Note (1): Indication of axis of galaxy studied:
     MJ = major axis and MN = minor axis
--------------------------------------------------------------------------------

Author's address:
    Claire Halliday    <ch@astro.livjm.ac.uk>

References:
    Bender, R. et al., 1989, A&A, 217, 35. (1989A&A...217...35B)
    Bender, R., 1990, A&A, 229, 441. (1990A&A...229..441B)
    de Vaucouleurs, G., de Vaucouleurs, A., Corwin, H.
         G.J., Buta, R.J., Paturel, G., Fouque, P., 1991, Third
         Reference Catalogue of Bright Galaxies. Springer Verlag (RC3)
         See Cat. <VII/155>
    Gerhard, O.E., 1993, MNRAS, 265, 213. (1993MNRAS..265..213G)
    Lauer, T.R., Ajhar, E.A., Byun, Y.-I., Dressler, A., Faber, S.M.,
         Grillmair, C., Kormendy, J., Richstone, D., Tremaine, S.
         1995, AJ, 110, 2622 (1995AJ....110.2622L)
    Peletier, R.F., Davies, R.L., Illingworth, G.D., Davis, L.E.,
         Cawson, M., 1990, AJ, 100, 1091. (1990AJ....100.1091P)
    Tonry, J., Dressler, A., Blakeslee, J. P., Ajhar, E. A.,
         Fletcher, A. B., Luppino, G. A., Metzger, M. R., Moore, C. B., 2001,
         ApJ, 546, 681 (2001ApJ...546..681T)
    van der Marel, R.P., Franx, M., 1993, ApJ, 407, 525
         (1993ApJ...407..525V)

Acknowledgements:
    The Digitized Sky Surveys were produced at the Space Telescope Science
    Institute under U.S. Government grant NAG W-2166.
================================================================================
(End)         Claire Halliday [Liverpool John Moores University]     10-Aug-2001

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