Spatial distribution of accreting isolated neutron stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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8 pages, 9 PostScript figures, to be presented as a poster at the conference "Current problems in astrophysics", Moscow, Septe

Scientific paper

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
$\approx 5 kpc$.

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