First detection of the growing humps at the rapidly rising stage of dwarf novae AL Com and WZ Sge

Astronomy and Astrophysics

Volumn 381, Issue 3, 2002, Pages

  Ishioka, R ^a   Uemura, M ^a   Matsumoto, K ^a,b   Ohashi, H ^a   Kato, T ^a   Masi, G ^c   Novak, R ^c   Pietz, J ^c   Martin, B ^c   Starkey, D ^c   Kiyota, S ^c   Oksanen, A ^c   Moilanen, M ^c   Cook, L ^c   Kral, L ^c   Hynek, T ^c   Kolasa, M ^c   Vanmunster, T ^c   Richmond, M ^c   Kern, J ^c   Davis, S ^c   Crabtree, D ^c   Beaulieu, K ^c   Davis, T ^c   Aggleton, M ^c   Gazeas, K ^c   Niarchos, P ^c   Yushchenko, A ^c   Mallia, F ^c   Fiaschi, M ^c   Good, G A ^c   Boyd, D ^c   Sano, Y ^c   Morikawa, K ^c   Moriyama, M ^c   Mennickent, R ^c   Arenas, J ^c   Ohshima, T ^c   Watanabe, T ^c   more..

^a KYOTO UNIVERSITY   (Japan)

^b OKAYAMA UNIVERSITY   (Japan)

^c VSNET Collaboration Team ^*

Author keywords

Stars: cataclysmic variables; Stars: dwarf novae; Stars: individual (WZ Sge)

Indexed keywords

LIGHT EMISSION; MASS TRANSFER; MATHEMATICAL MODELS; PHOTOMETRY; SPACE RESEARCH;

DWARF STARS;

ASTRONOMY;

EID: 0036188501     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20011644     Document Type: Article

References (22)