A nova-like red variable in M31

Details A nova-like red variable in M31 A nova-like red variable in M31

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...353l..35m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 353, April 20, 1990, p. L35-L37.

Astronomy and Astrophysics

Astrophysics

46

Andromeda Galaxy, Late Stars, Novae, Red Giant Stars, Supergiant Stars, Variable Stars, Bolometers, M Stars, Stellar Magnitude, Stellar Spectra

Scientific paper

A late-type supergiant which appeared in the bulge of M31 in the last
observing season faded 3 bolometric magnitudes in 100 days and is now no
longer detectable. It is suggested that the object was a nova of an
unusual type.

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