Spatial distribution of accreting isolated neutron stars
arXiv:astro-ph/9609126 · doi:10.1023/A:1000869123628
Abstract
We present here the computer model of the distribution of the luminosity, produced by old isolated neutron stars (OINSs) accreting from the interstellar medium (ISM). We show, that for different mean velocities of OINSs the distribution of the luminosity has a torus-like structure, with the maximum at .
8 pages, 9 PostScript figures, to be presented as a poster at the conference "Current problems in astrophysics", Moscow, September 23-28, 1996. Short version will be published in Astronomical and Astrophysical Transactions