The problem of the high mass of the hot component in the recurrent nova T Coronae Borealis solved after 38 years

Astronomy and Astrophysics

Volumn 339, Issue 2, 1998, Pages 449-456

  Hric, I ^a   Petrik K ^b   Urban, Z ^a   Niarchos, P ^c   Anupama, G C ^d  

^a ASTRONOMICAL INSTITUTE   (Slovakia)

^b TRNAVA UNIVERSITY   (Slovakia)

^c UNIVERSITY OF ATHENS   (Greece)

^d INDIAN INSTITUTE OF ASTROPHYSICS   (India)

Author keywords

Novae, cataclysmic variables; Stars: individual: T CrB; White dwarfs

Indexed keywords

EID: 0039993626     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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