Integrated Radio Luminosities of Pulsars (Malov+, 2006)

Details Integrated Radio Luminosities of Pulsars (Malov+, 2006) Integrated Radio Luminosities of Pulsars (Malov+, 2006)

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..90830542m&link_type=abstract

VizieR On-line Data Catalog: J/AZh/83/542. Originally published in: 2006AZh...83...542M; 2006ARep..50...483M

Computer Science

Pulsars, Radio Sources

Scientific paper

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. . 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.
(2 data files).

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