Astronomical Data Center

ADCADC/CDS Standard Document for Catalog:
/catalogs/7/7103/

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


VII/103     Galactic Globular Clusters (Monella 1985)
================================================================================
Catalogue of Galactic Globular Clusters
    Monella R.
    <Coelum LIII, 287 (1985)>
================================================================================
ADC_Keywords: Clusters, globular 

Description:
   The catalogue collects, for the first time, the most important data 
   concerning all the galactic globular clusters still well known. 
   Here the objects enclosed in famous publications like the ones of Arp 
   (1965), Alter et al. (1970), Alcaino (1973) are reported,
   with the addition of new clusters noticed recently (TER, ESO, UKS, TJ)
   and till KOD 1, found by K. Kodaira in July 1983 (IAUC 3846).
   The most important disposable data in literature have been found about 
   every object. For the clusters found recently, the data may be 
   fragmentary and susceptible of variations. A particular care has been 
   utilized in the research of the most reliable informations and data, 
  that have been homogenized and put in order later on.

File Summary:
--------------------------------------------------------------------------------
 FileName       Lrecl  Records   Explanations
--------------------------------------------------------------------------------
ReadMe             80        .   This file
catalog.dat       120      161   Catalog Data
--------------------------------------------------------------------------------

Byte-by-byte Description of file: catalog.dat
--------------------------------------------------------------------------------
   Bytes Format  Units   Label    Explanations
--------------------------------------------------------------------------------
   2-  4  I3     ---     ID       [1,160]+ Running number
   7-  9  A3     ---     Constel  Constellation of belonging
  12- 21  A10    ---     Name     Common name of the globular cluster
  24- 25  I2     h       RAh      Right Ascension 1950 (hours)
  27- 28  I2     min     RAm      Right Ascension 1950 (minutes)
  30- 31  I2     s       RAs      [0/60[? Right Ascension 1950 (seconds)
      33  A1     ---     DE-      Declination 1950 (sign)
  34- 35  I2     deg     DEd      Declination 1950 (degrees)
  37- 40  F4.1   arcmin  DEm      Declination 1950 (minutes)
  43- 47  F5.2   mag     V        ? Photovisual apparent integrated magnitude
  49- 54  F6.2   mag     Mv       ? Photovisual absolute integrated magnitude
  56- 60  A5     ---     Sp       Spectral integrated class
  63- 67  F5.2   ---     [Fe/H]   ? Degree of metallicity
  70- 74  F5.2   arcmin  AppDiam  ? Photographic apparent diameter
  76- 80  F5.1   pc      RealDiam ? Real diameter
  84- 87  F4.1   mag     m(BS)    ? Apparent magnitude of the brightest star
  89- 95  F7.3   kpc     d-galaxy ? Distance from the center of our Galaxy
  97-103  F7.3   kpc     d-sun    ? Distance from Sun
 105-108  A4     ---     ConClas  Concentration class according to Sawyer-Hogg
 110-113  I4     km/s    RV       ? Radial velocity
 115-117  I3     ---     N(var)   ? Number of var. stars found in the cluster
 118-120  A3     ---     Note     (?)
--------------------------------------------------------------------------------
Historical note: 
  The distance d of cluster#8 was corrected from 16.4 to 116.4kpc to agree 
  with the publication.

Author:
     R. MONELLA
     Sharru Astronomical Observatory, Via Giovanni XXIII, 13,
     24050   COVO (Bergamo), Italy

References:
  Arp, H. 1965, ApJ, 141, 43
  Alcaino, G. 1974, A&AS, 13, 55  
  Alcaino, G. 1974, A&AS, 18, 9
================================================================================
(End) Francois Ochsenbein [CDS]; C.-H. Joseph Lyu [Hughes STX/NASA]  26-Sep-1996

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