Distribution of the luminosity of accreting isolated compact objects
classification
🌌 astro-ph
keywords
luminosityaccretingdistributionisolatedapproxblackcompactcomputer
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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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