The 2000-2001 superoutburst of the WZ Sge-type star RZ Leonis: A clue to understanding the origin of viscosity in quiescent dwarf nova disks

Publications of the Astronomical Society of Japan

Volumn 53, Issue 5, 2001, Pages 905-913

  Ishioka, Ryoko ^a   Kato, Taichi ^a   Uemura, Makoto ^a   Iwamatsu, Hidetoshi ^a   Matsumoto, Katsura ^a   Stubbings, Rod ^b   Mennickent, Ronald ^c   Billings, Gary W ^b   Kiyota, Seiichiro ^d   Masi, Gianluca ^b   Pietz, Jochen ^b   Novak, Rudolf ^e   Martin, Brian E ^f   Oksanen, Arto ^g   Moilanen, Marko ^g   Torii, Ken'ichi ^h   Kinugasa, Kenzo ⁱ   Kawakita, Hideyo ⁱ  

^a KYOTO UNIVERSITY   (Japan)

^b Universidad de Concepcion ^*

^c UNIVERSITY OF CONCEPCIÓN   (Chile)

^d Center for Balcony Astrophysics   (Japan)

^e N Copernicus Observatory and Planetarium   (Czech Republic)

^f KING S UNIVERSITY COLLEGE   (Canada)

^g Astronomical Association Jyväskylän Sirius   (Finland)

^h INST OF PHYS AND CHEMICAL RESEARCH   (Japan)

ⁱ Gunma Astronomical Observatory   (Japan)

Author keywords

Stars: cataclysmic variables; Stars: dwarf novae; Stars: individual (RZ Leo)

Indexed keywords

STARS;

CATACLYSMIC VARIABLES; DWARF NOVAE; LONG DURATION; PHOTOMETRICS; STAR: CATACLYSMIC VARIABLE; STAR: INDIVIDUAL (RZ LEO); STARS: DWARF NOVAE; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:CATACLYSMIC; TIME-RESOLVED;

VISCOSITY;

EID: 0035541464     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/53.5.905     Document Type: Article

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