Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...321..447p&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 321, Oct. 1, 1987, p. 447-449.
Astronomy and Astrophysics
Astrophysics
47
Pulsars, Spectral Energy Distribution, Stellar Models, Visible Spectrum, X Ray Stars
Scientific paper
The optical luminosity of PSR 0540 is considerably stronger than what one would have predicted in a simple model developed earlier where the pulses are synchrotron radiation by secondary electrons near the light cylinder. This discrepancy can be eliminated if one incorporates into the model the effects of the large duty cycle and the spectral properties of PSR 0540. The authors also show that the same model can provide a reasonable fit to the observed X-ray fluxes from fast pulsars.
Pacini Franco
Salvati Marco
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