[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-alert 6178] Re: WZ Sge: superhumps likely evolving
- Date: Fri, 03 Aug 2001 04:45:49 +0200 (CEST)
- To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- From: gian.masi@flashnet.it
- Subject: [vsnet-alert 6178] Re: WZ Sge: superhumps likely evolving
- Cc: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign@kusastro.kyoto-u.ac.jp, vsnet-superoutburst@kusastro.kyoto-u.ac.jp
- In-Reply-To: <200108030235.LAA18235@ceres.kusastro.kyoto-u.ac.jp>
- References: <200108030235.LAA18235@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
- User-Agent: Cybernet Italia Webmail
Dear Taichi,
thank you very much for your kind comment.
Hopefully, I will have my data (from this last night!)
reduced and on their way to you in one hour or so (882/1260
images reduced right now).
It looks like as another important as exciting observing
season is just starting.
Regards,
Gianluca
CBA - VSNET Collaboration team
>
> Oh, thanks for the comment. The "nominal" period (as
inferred from
> the
> period analysis) is now shorter than the orbital period.
This may be
> called
> as "negative superhumps", but my interpretation is that
the true
> superhump
> signal is rising at a smaller phase than in early
superhumps. The net
> effect
> seems to be observed as a "shortening of the mean period".
I will
> make
> a more detailed analysis, using a longer baseline
observations later.
>
> Regards,
> Taichi Kato
> VSNET Collaboration team
>
>
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp