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1998A&A...339..449H - Astronomy and Astrophysics, volume 339, 449-456 (1998/11-2)
The problem of the high mass of the hot component in the recurrent nova T Coronae Borealis solved after 38 years.
HRIC L., PETRIK K., URBAN Z., NIARCHOS P. and ANUPAMA G.C.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): stars: individual: T CrB - novae, cataclysmic variables - white dwarfs
Simbad objects: 1
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