Optically thick wind solutions for an extremely rapid light curve of recurrent novae

Publications of the Astronomical Society of Japan

Volumn 51, Issue 4, 1999, Pages 525-535

  Kato, Mariko ^a  

^a KEIO UNIVERSITY   (Japan)

Author keywords

Stars: individual (U Scorpii, V394 Coronae Australis, T coronae Borealis, V745 Scorpii); Stars: mass loss; Stars: Novae; Stars: Population II; Stars: white dwarfs

Indexed keywords

CHEMICAL ELEMENTS; CURVE FITTING;

BOREALIS; FISH-EYE; LIGHT CURVES; MASS LOSS; STAR: INDIVIDUAL (U SCORPII, V394 CORONA AUSTRALI, T CORONA BOREALI, V745 SCORPII); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: MASS-LOSS; STARS: POPULATION II; STARS: WHITE DWARF; STARS:NOVAE; HEAVY ELEMENTS; STAR: INDIVIDUAL (U SCORPII V394 CORONA AUSTRALI T CORONA BOREALI V745 SCORPII);

WHITE DWARFS;

EID: 0033465882     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/51.4.525     Document Type: Article

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