Distribution of the luminosity of accreting isolated compact objects

Details Distribution of the luminosity of accreting isolated compact objects Distribution of the luminosity of accreting isolated compact objects

1997-05-29

arxiv.org/abs/astro-ph/9705236v2

A&A V. 331, p.535 (1998)

Astronomy and Astrophysics

Astrophysics

4 pages, 6 PostScript figures. Uses l-aa style. To be presented as a poster at the conference "Neutron stars - 97", St. Peters

Scientific paper

We present here the computer model of the distribution of the luminosity,
produced by old isolated neutron stars and black holes accreting from the
interstellar medium in the Galaxy in R-Z plane. We show, that the luminosity
distributions have a torus-like structure, with the maximum at $\approx 5-6
kpc$.

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