The supernovae near the nuclei of M31 and the Galaxy

Details The supernovae near the nuclei of M31 and the Galaxy The supernovae near the nuclei of M31 and the Galaxy

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...265..719v&link_type=abstract

Astrophysical Journal, Part 1, vol. 265, Feb. 15, 1983, p. 719-721.

Mathematics

Probability

4

Andromeda Galaxy, Galactic Nuclei, Milky Way Galaxy, Supernova Remnants, Abundance, Binary Stars, Galactic Structure, Metallic Stars, Nebulae, Stellar Evolution

Scientific paper

The fact that the supernova remnant Sgr A East is quite small suggests that it is fairly young (not greater than approximately 6800 yr). The a priori probability that a supernova should have occurred so recently within about 2.5 pc of the galactic nucleus is calculated to be not greater than approximately 0.1. The a priori probability that a supernova such as S And would have occurred within 16 arcsec of the nucleus of M31 is found to be approximately 0.005. Such low probabilities suggest the remote possibility that the occurrence of these supernovae might, in some unspecified way, be related to their proximity to galactic nuclei.

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