Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984atsir1349....1o&link_type=abstract
Astronomicheskii Tsirkulyar NO.1349/NOV16, 1985
Astronomy and Astrophysics
Astronomy
1
Scientific paper
As it has been shown earlier, both the H I+He I wind and a significant part of the total radiation of the IRS 16 centre can be attributed to a superstar (SS) of the mass ≡ 300 M_sun;, while both gamma continuum radiation and positrons for the 0.511 MeV annihilation line from the galactic centre can be most naturally explained by a moderate-mass black hole (MMBH) of the mass 10 - 300 M_sun;. It is argued that, if the IRS 16 centre is spatially separated from the compact radio source Sgr A, the symbiotic object consisting of an SS and an MMBH seems to be able to explain the most principal features of the galactic centre emission.
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