Distribution of the luminosity of accreting isolated compact objects

Abstract

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 $\approx 5-6kpc$.

arXiv comment4 pages, 6 PostScript figures. Uses l-aa style. To be presented as a poster at the conference "Neutron stars - 97", St. Petersburg, June 9-11, 1997. In the replaced version fig. 3 and 5 are changed