THE OBSERVED INTEGRAL RADIO LUMINOSITIES OF 232 PULSARS

Authors
MALOV IF MALOFEEV VM SENE DS
Citation
If. Malov et al., THE OBSERVED INTEGRAL RADIO LUMINOSITIES OF 232 PULSARS, ASTRONOM ZH, 71(5), 1994, pp. 762-767
Citations number
20
Categorie Soggetti
Astronomy & Astrophysics
Journal title
ASTRONOMICESKIJ ZURNAL
ISSN journal
00046299 → ACNP
Volume
71
Issue
5
Year of publication
1994
Pages
762 - 767
Database
ISI
SICI code
0004-6299(1994)71:5<762:TOIRLO>2.0.ZU;2-8
Abstract
The integral radio luminosities of 232 pulsars are calculated on the b ase of the analysis of new data about the mean spectra. For 88% of the pulsars, the values of the luminosities lie in the range of 10(27) - 10(30) erg/s. It is shown that the pulsar luminosity remains constant over a period of a few million years. The mean power of the radiation increases with the period P as P0.5. The increasing of the luminosity with the rate of loss of the rotational energy is revealed.