Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/journal_tables/A+A/296/643/

The following is the "ReadMe" document that describes this ADC catalog. You can access the files described here in three ways:

1. Use the ADC Data Viewer Suite to visualize the data. [preview
2. Get the data files via anonymous FTP. (See Note.) [ftp


J/A+A/296/643    Low Surface Brightness galaxies in Coma   (Karachentsev+ 1995)
================================================================================
A search for low surface brightness dwarf galaxies in the Coma cluster core
     Karachentsev I.D., Karachentseva V.E., Richter G.M., Vennik J.A.
    <Astron. Astrophys. 296, 643 (1995)>
    =1995A&A...296..643K      (SIMBAD/NED BibCode)
================================================================================
ADC_Keywords: Clusters, galaxy ; Galaxies, photometry
Keywords: Coma cluster - galaxies: dwarf - galaxies: general

Abstract:
    Using the prime focus of the 6-meter telescope, we have searched for
    low surface brightness dwarf galaxies in two regions in the Coma
    cluster: one in the center of the cluster and the other one 40arcmin
    to the west. The observations were carried out with a total exposure
    time 4x5x600sec and with a 1.2arcsec seeing. Our survey is complete
    down to V=25.5 and R=25.0mag. The central field shows an excess of
    faint galaxies (121 versus 104 in the reference field) significant at
    a one sigma level only. However, the central-field excess is mainly
    caused by the presence of faint (V=24/25mag), neutral colour
    (V-R=0.3/0.4) objects of low surface brightness,
    SB=26.0/26.5mag/arcsec^2^. These characteristics are quite consistent
    with those of the dwSph's in the Local Group which have typically
    M_v_~10mag and A~1kpc. The observed excess corresponds to a surface
    number density of 4gal/arcmin^2^ in the center of Coma, thus implying
    a total population of cluster dwarfs of ~4000 down to the limiting
    absolute magnitude -10mag. The number ratio of LSBD's to normal
    galaxies (with M<-18mag for normals) in Coma turns out to be 20:1.
    Such ratio is comparable to that observed in other rich clusters:
    A3574 (14:1) and A1367 (6:1), but is much larger than the 2:1 ratio
    obtained for moderate nearby clusters such as Virgo, Fornax, Antlia.

Objects:
    -----------------------------------------
       RA   (2000)   DE    Designation(s)
    -----------------------------------------

File Summary:
--------------------------------------------------------------------------------
  FileName      Lrecl  Records  Explanations
--------------------------------------------------------------------------------
ReadMe             80        .  This file
table1             46      121  Properties of galaxies in the central Coma field
table2             46      104  Properties of galaxies in the reference field
--------------------------------------------------------------------------------

Byte-by-byte Description of file: table1 table2
--------------------------------------------------------------------------------
   Bytes Format Units      Label     Explanations
--------------------------------------------------------------------------------
   1-  3  I3    ---        ID        Galaxy identification number
   5-  9  F5.2  mag        Vmag      Apparent total V magnitude
  11- 15  F5.2  mag        Rmag      Apparent total R magnitude
  17- 20  F4.1  arcsec     DiamV     Angular diameter measured on V frame
  22- 25  F4.1  arcsec     DiamR     Angular diameter measured on R frame
  27- 31  F5.2  mag/arcsec SBV       Average surface brightness within DiamV
  33- 37  F5.2  mag/arcsec SBR       Average surface brightness within DiamR
  39- 43  F5.2  mag        V-R       Total V-R color index
  45- 46  A2    ---        Note      Notes (1)
--------------------------------------------------------------------------------
Note (1): bn: binary image
          df: diffuse object without a marked brightness gradient
          st: star-like image
--------------------------------------------------------------------------------

History: Prepared via OCR at CDS.
================================================================================
(End)                           James Marcout, Patricia Bauer [CDS]  07-Mar-1997

Go to ADC Home Page