New Approach to Sgr A* Problem

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dc.creatorVerozub, L.
dc.date2002-01-18
dc.date.accessioned2026-07-07T02:02:17Z
dc.date.available2026-07-07T02:02:17Z
dc.descriptionThe hypothesis that radiation of Sgr A* is caused by accretion onto a supermassive compact object without the events horizon is studied. The main equations of the accretion and a relativistic equation of the trasfer radiation are obtained. The synchrotron spectrum in the vicinity of the maximum is considered.
dc.description9 pages, 3 figures, LaTeX2e
dc.identifierhttps://arxiv.org/abs/astro-ph/0201316
dc.identifierhttp://arxiv.org/abs/astro-ph/0201316
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4034
dc.subjectAstrophysics
dc.titleNew Approach to Sgr A* Problem
dc.typetext

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