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[vsnet-chat 2006] Re: Correction: NY Ser humps
- Date: Mon, 21 Jun 1999 20:06:36 -0700 (PDT)
- To: jop@astro.colombia.edu, Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Lew Cook <lcoo@yahoo.com>
- Subject: [vsnet-chat 2006] Re: Correction: NY Ser humps
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Joe Patterson has several other sets of data and he
tells me that he has identified the superhump period
at 0.1042+-.0003 d.
Maybe he has a comment.
Regards, Lew
--- Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> wrote:
> Re: [vsnet-chat 2004] Re: Correction: NY Ser humps
>
> > A nice fit. The period of 0.1037 is shorter than
> Taichi Kato
> > mentions. I know that on VW Hydri the SH period
> shortens during the
> > outburst but it's about 20 years since I took much
> interest in SH periods
> > on SU UMa stars.
>
> I hope the very Nogami-san may have some comment
> on the previously
> measureed superhump period of NY Ser.
>
> Superhump periods of textbook SU UMa stars
> decrease during superoutburst,
> usually at a rate of Pdot/P = 10^{-6}. However,
> recent observations indicate
> some of short-period SU UMa stars show (best
> examples being SW UMa, V1028 Cyg,
> AL Com, V485 Cen) positive Pdots. The inferred
> period may be suggestive
> of a negative Pdot (as in usual SU UMa stars), more
> observations and analysis
> may be needed to verify the actually shortening.
>
> Regards,
> Taichi Kato
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