How is Binary Radio-Pulsars with Black Holes Population Rich?

Details How is Binary Radio-Pulsars with Black Holes Population Rich? How is Binary Radio-Pulsars with Black Holes Population Rich?

2005-03-16

arxiv.org/abs/astro-ph/0503341v1

Mon.Not.Roy.Astron.Soc. 359 (2005) 1517-1523

Astronomy and Astrophysics

Astrophysics

8 pages, 4 figures, accepted to MNRAS

Scientific paper

10.1111/j.1365-2966.2005.08997.x

Using "Scenario Machine" we have carried out population synthesis of radio pulsar with black hole binaries (BH+Psr) in context of the most wide assumptions about star mass loss during evolution, binary stars mass ratio distribution, kick velocity and envelope mass lost during collapse. Our purpose is to display that under any suppositional parameters of evolution scenario BH+Psr population have to be abundant in Galaxy. It is shown that in the all models including models evolved by Heger et al. (2002), Woosley et al. (2002), Heger et al. (2003) expected number of the black holes paired with radio pulsars is sufficient enough to discover such systems within the next few years.

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