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[vsnet-alert 397] a New SU UMa Star, PG1510+234
- Date: Wed, 24 Apr 1996 07:21:35 +0900
- To: vsnet-alert
- From: Daisaku Nogami <nogami>
- Subject: [vsnet-alert 397] a New SU UMa Star, PG1510+234
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear Colleagues,
Our observation revealed that the ongoing outburst in PG 1510+234
(=NSV06990 = Ser1 in Downes & Shara(1993)) has been lasting for at
least three days and the superhumps with an amplitude of ~0.3 mag
clearly exist on April 23. Although the superhump period can not
be measured precisely due to shortness of the coverage, it seems
to exceed 2 hours. It was proved that PG 1510+234 is an SU UMa-type
dwarf nova with a small amplitude of ~3mag.
Best regards,
Daisaku Nogami & Ouda Team
Return to Daisaku Nogami
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