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[vsnet-alert 2959] NY Ser more information
- Date: Mon, 10 May 1999 10:13:52 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 2959] NY Ser more information
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
NY Ser more information
Additional information on this target, extracted from previous vsnet-alert
messages:
-----------------------------------------------------------------------------
(vsnet-alert 397, 1996 Apr. 23)
> 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
(vsnet-alert 398)
> Dear Colleagues,
>
> We have just reduced the PG1510+234 data obtained in the last
> night. The superhumps with an amplitude of ~0.3 mag still
> existed. Surprisingly, our period analysis using the April 23
> and 24 results gives the superhump period of 0.1064 (+-0.0003)
> day (= 153.2 (+-0.4) min)! Is PG 1510+234 located at the midst
> of the CV period gap?!
>
> Best regards,
> Daisaku Nogami & Ouda Team
-----------------------------------------------------------------------------
The full paper, with detailed long-term photometry, by D. Nogami et al.
is available at
http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/preprints/NY_Ser
and the preceding paper on outburst activity information
http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/preprints/PG1510+234
VSNET NY Ser page:
http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/pg1510.html
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp