Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-03-21
Astron.Astrophys.358:617-623,2000
Astronomy and Astrophysics
Astrophysics
8 pages, 4 figures. Accepted for publication in A&A Main Journal
Scientific paper
We analyzed the power density spectra of a sample of 9 neutron star and 9 black hole binaries in the low/hard spectral state. In the power density spectra of accreting neutron stars with a weak magnetic field a significant power is contained at frequencies close to one kHz. At the same time, most Galactic accreting black holes demonstrate a strong decline in the power spectra at the frequencies higher than 10--50 Hz. We propose to use this empirical fact as a method to distinguish the accreting neutron stars from black holes in X-ray transients. The X-ray transients that demonstrate significant noise in their X-ray flux at frequencies above ~500 Hz should be considered neutron stars. We propose to explain the observed difference as a result of the existence of a radiation dominated spreading layer on the neutron star surface (Inogamov & Sunyaev 1999). The possible very high frequency variabilities of this layer are discussed.
Revnivtsev Mike
Sunyaev Rachid
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