A supernova in NGC 1199

Details A supernova in NGC 1199 A supernova in NGC 1199

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....93...53l&link_type=abstract

Astronomy and Astrophysics, vol. 93, no. 1-2, Jan. 1981, p. 53.

Astronomy and Astrophysics

Astrophysics

Elliptical Galaxies, Supernovae, Electronography

Scientific paper

A faint stellar object was detected in NGC 1199 elliptical galaxy which was interpreted as a supernova explosion. Since it is known that only type I supernovae occur in elliptical galaxies, the color indices of this type were used to derive the value for the intensity B equals 20.4 plus or minus 0.2; using the galactic absorption magnitude of 0.26 (de Vaucouleurs, 1976), B is equal to 20.1 plus or minus 0.2, with the absolute magnitude of -11.9. This shows that the supernova has already significantly decreased since its maximum.

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