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 2006AZh...83...542M
=2006ARep..50...483M 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:
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FileName Lrecl Records Explanations
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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)
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See also:
VII/189 : Catalog of Pulsars (Taylor+, 1995)
Byte-by-byte Description of file: table*.dat
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Bytes Format Units Label Explanations
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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
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(End) Veta Avedisova [INASAN] 01-Jul-2007