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Photometric study of new southern SU UMa-type dwarf novae and candidates: V877 Ara, KK Tel and PU CMa
Authors:Taichi Kato  Roland Santallo  Greg Bolt  Tom Richards  Peter Nelson  Berto Monard  Makoto Uemura  Seiichiro Kiyota  Rod Stubbings  rew Pearce  Tsutomu Watanabe  Patrick Schmeer  Hitoshi Yamaoka
Affiliation:Department of Astronomy, Faculty of Science, Kyoto University, Sakyo-ku, Kyoto 606-8502, Japan;Southern Stars Observatory, PO Box 60972, 98702 Faaa Tahiti, French Polynesia;295 Camberwarra Drive, Craigie, Western Australia 6025, Australia;Woodridge Observatory, 8 Diosma Road, Eltham, Victoria 3095, Australia;RMB 2493, Ellinbank, Victoria 3820, Australia;Bronberg Observatory, PO Box 11426, Tiegerpoort 0056, South Africa;Variable Star Observers League in Japan (VSOLJ), 1-401-810 Azuma, Tsukuba 305-0031, Japan;19 Greenland Drive, Drouin, Victoria 3818, Australia;32 Monash Avenue, Nedlands, Western Australia 6009, Australia;Variable Star Observers League in Japan (VSOLJ), 117 Shirao Dormitory, 1414 Oonakazato, Shizuoka 418-0044, Japan;Bischmisheim, Am Probstbaum 10, 66132 Saarbrücken, Germany;Faculty of Science, Kyushu University, Fukuoka 810-8560, Japan
Abstract:
Keywords:accretion  accretion discs  stars: dwarf novae  stars: individual: KK Tel  stars: individual: PU CMa  stars: individual: V877 Ara  novae  cataclysmic variables
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