TV Corvi revisited: Precursor and superhump period derivative linked to the disk instability model

Astronomy and Astrophysics

Volumn 432, Issue 1, 2005, Pages 261-271

  Uemura, M ^a,b   Mennickent, R E ^a   Ishioka, R ^c   Imada, A ^c   Kato, T ^c   Nogami, D ^c   Stubbings, R ^d   Kiyota, S ^e   Nelson, P ^d   Tanabe, K ^f   Heathcote, B ^g   Bolt, G ^d  

^a UNIVERSITY OF CONCEPCIÓN   (Chile)

^b KYOTO UNIVERSITY   (Japan)

^c KYOTO UNIVERSITY   (Japan)

^d RMB 2493 ^*  (Australia)

^e Variable Star Observers League Japan   (Japan)

^f OKAYAMA UNIVERSITY OF SCIENCE   (Japan)

^g Barfold Observatory   (Australia)

Author keywords

Accretion, accretion disks; Binaries: close; Novae, cataclysmic variables; Stars: dwarf novae; Stars: individual: TV Crv

Indexed keywords

COMPUTER SIMULATION; COSMIC RAYS; ELECTROMAGNETIC WAVE PROPAGATION; EXTRATERRESTRIAL ATMOSPHERES; HYDRODYNAMICS; PHOTOMETRY;

ACCRETION DISKS; BINARIES: CLOSE; CATACLYSMIC VARIABLES; NOVAE; STARS: DWARF NOVAE; STARS: INDIVIDUAL: TV CRV;

ASTRONOMY;

EID: 20044374168     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20042004     Document Type: Article

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