Light curve of the peculiar supernova 1985f in NGC 4618

Details Light curve of the peculiar supernova 1985f in NGC 4618 Light curve of the peculiar supernova 1985f in NGC 4618

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..784t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Oct. 1986, p. 784-788) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Sept.-Oc

Astronomy and Astrophysics

Astronomy

7

Light Curve, Peculiar Stars, Stellar Luminosity, Stellar Spectrophotometry, Supernovae, Spectrum Analysis, Stellar Magnitude

Scientific paper

Observations of SN 1985f obtained with the 40-cm astrograph and 70-cm reflector of the Shternberg Astronomical Institute at Moscow are examined. The B,V magnitude of the star is studied and compared with the magnitudes of other supernovae. Analysis of the SN 1985f light curve reveals that the point of maximum light was 12.1 mag + or - 0.1 mag on June 12, 1984, and the curve resembles that of type 1 supernovae, in particular 1962l, 1963j, and 1976b. The absolute magnitude of the star was calculated as ranging from -17.6 to -19.1 mag.

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