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J/AZh/83/542        Integrated Radio Luminosities of Pulsars      (Malov+, 2006)
Integrated Radio Luminosities of Pulsars.
    Malov I.F., Malov O.I.
   <Astron. Zh. 83, 542 (2006)>
   =2006AZh...83...542M
   =2006ARep..50...483M
ADC_Keywords: Pulsars; Radio sources


Abstract:
    The integrated radio luminosities of 311 long-period (P>0.1s) and
    27 short-period (P<0.1s) pulsars have been calculated using a new
    compilation of radio spectra. The luminosities are in the range
    1027-1030erg/s for 88% of the long-period pulsars and
    1028-1031erg/s for 88% of the short-period pulsars. We find a high
    correlation between the luminosity L and the estimate L1=S(400)*d2
    from the catalog of Taylor et al. (1993, See Cat. VII/189. The
    factor 'eta' for transformation of the rotational energy of the
    neutron star into radio emission increases/decreases with increasing
    period for long-period/short-period pulsars. The mean value of
    'eta'=-3.73 for the long-period and -4.85 for the short-period
    pulsars.

File Summary:

       FileName      Lrecl  Records   Explanations

ReadMe            80        .   This file
table2.dat        23       27   Luminosities of short-period pulsars (P<0.1s)
table3.dat        23      311   Luminosities of long-period pulsars  (P>0.1s)


See also:
     VII/189 : Catalog of Pulsars (Taylor+, 1995)


Byte-by-byte Description of file: table*.dat

   Bytes Format  Units    Label    Explanations

   1-  3  I3     ---      Seq      Running number
   6- 16  A11    ---      Name     Name of pulsar
  19- 23  F5.2   [10-7W]  logL     Log of luminosity in erg/s

(End)                    Veta Avedisova [INASAN]                     01-Jul-2007