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[vsnet-alert 7590] Var73 Dra: first ER UMa-like dwarf nova in the period gap?
- Date: Tue, 10 Dec 2002 15:42:04 +0900 (JST)
- To: vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp, vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp, vsnet-superoutburst@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 7590] Var73 Dra: first ER UMa-like dwarf nova in the period gap?
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
Var73 Dra: first ER UMa-like dwarf nova in the period gap?
Donn Starkey's most recent observation almost certainly confirms that
the present outburst is a superoutburst(!). This finding suggests that
the minimum supercycle length of Var73 Dra is around ~60 d (or possibly
slightly shorter). This shortness of the supercycle is comparable to
those of ER UMa-type dwarf novae. In conjunction with Antipin and Pavlenko
(2002) A&A 391, 565, the supercycle of this object may not be as stable
as in ER UMa stars. Such a variation of the supercycles was also
recorded in the in-the-gap SU UMa-type dwarf nova, NY Ser (Nogami et al.
1998, PASJ 50, L1).
Further observations of Var73 Dra during the present outburst is
planned. We also strongly encourage multi-longitude observations to
compensate the short visibility in this season.
Regards,
Taichi Kato
VSNET Collaboration team
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp