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[vsnet-alert 5441] RZ Leo: most recent outbursts
- Date: Wed, 20 Dec 2000 20:48:22 +0100
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, Patrick Schmeer <extpasc@mars.rz.uni-sb.de>
- From: Patrick Schmeer <extpasc@rz.uni-sb.de>
- Subject: [vsnet-alert 5441] RZ Leo: most recent outbursts
- In-Reply-To: <200012201733.CAA16780@ceres.kusastro.kyoto-u.ac.jp>; from tkato@kusastro.kyoto-u.ac.jp on Thu, Dec 21, 2000 at 02:33:03AM +0900
- References: <200012201733.CAA16780@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
On Thu, Dec 21, 2000 at 02:33:03AM +0900, Taichi Kato wrote in
[vsnet-alert 5438]:
> RZ Leo: call for immediate follow-up observations!
>
> As reported by Rod Stubbings in [vsnet-alert 5437], the possible WZ Sge
> type dwarf nova RZ Leo is undergoing an extremely rare outburst!
> Despite a number of unconfirmed possible sighting reports, the last
> time when the outburst of this star was observed dates back to 1987!
On 1989 Mar. 10.9 UT I observed RZ Leo at mv= 13.5 - that one was probably a
normal outburst (see also IAUC 4757).
On 1990 Oct. 27 Gerald Dyck made a 12.8 mag estimate - apparently another
normal outburst.
The last recorded (likely) superoutburst occurred on 1987 Nov. 28 (cf. IAUC
4504).
On the basis of the last four recorded outbursts I get a mean cycle length
of 527 days. The supercycle may be 13 years!
Regards,
Patrick
P.S.:
RZ Leo is one of the top-priority objects on my program. Unfortunately I
could not observe this likely SU UMa-type dwarf nova the last days due to
overcast skies.
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