Nova rate in the Local Group galaxies

Details Nova rate in the Local Group galaxies Nova rate in the Local Group galaxies

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993astl...19..147s&link_type=abstract

Astronomy Letters, Vol. 19, p. 147-152; Pis'ma v Astronomicheskij Zhurnal (ISSN 0320-0108), vol. 19, no. 5, p. 387-400. In Russ

Astronomy and Astrophysics

Astronomy

3

Andromeda Galaxy, Frequency Distribution, Local Group (Astronomy), Spiral Galaxies, Stellar Mass Ejection, Supernovae, Galactic Bulge, Infrared Astronomy, Light Curve, Stellar Luminosity

Scientific paper

Nova rates in the disk of M 31, its companions M 32 and NGC 205, as well as in M 33 are estimated on the basis of observational data obtained in the Crimea and Latvia during 1967-1990. The new data confirm a significant difference between the specific nova rates in the disk and in the bulge of M 31 (rhoB = 24.4-35.1). Similar results are obtained using galactic luminosities in the infrared K band.

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