On the constancy of the absolute magnitude MB /15/ of a classical nova 15 days after maximum light

Details On the constancy of the absolute magnitude MB /15/ of a classical nova 15 days after maximum light On the constancy of the absolute magnitude MB /15/ of a classical nova 15 days after maximum light

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...243..268s&link_type=abstract

Astrophysical Journal, Part 1, vol. 243, Jan. 1, 1981, p. 268-270. Research supported by the National Research Council of Canad

Astronomy and Astrophysics

Astrophysics

17

Astrometry, Novae, Stellar Magnitude, Stellar Luminosity, Time Response, White Dwarf Stars

Scientific paper

The absolute blue magnitudes of novae are predicted to have minimum spread approximately 18 days after visual maximum, in good agreement with the empirically determined value of 15 days. The absolute blue magnitude (15) is derived theoretically from the recently explained MB - t3 relation for novae; it is a slowly varying function of t3 (the time to decline 3 mag from maximum), which agrees well with observations.

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