Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7529971i&link_type=abstract
Why are there so few X-ray stars? NASA Transl. into ENGLISH from Russian report Pr-202, 1974 p 1-32
Astronomy and Astrophysics
Astronomy
Binary Stars, Radiation Sources, X Ray Sources, Black Holes (Astronomy), Neutron Stars, Roche Limit, Stellar Winds
Scientific paper
Conditions are discussed under which a binary star can be converted into a source of X-ray radiation depending on the condition under which stellar wind accretion of matter in the form of a disk can occur on a black hole or neutron star. It is shown that the main condition for the appearance of an X-ray source in a binary system is that the dimensions of its normal component be close to the dimensions of its Roche's cavity. It was found that old isolated pulsars cannot become sources of ultraviolet and soft X-ray radiation.
Illarionov Andrei F.
Syunyayev R. A.
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