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[vsnet-chat 3934] Re: [vsnet-campaign-nova 123] Re: Possible Nova in Pup
- Date: Wed, 3 Jan 2001 02:03:21 +0000 (GMT)
- To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- From: "<Dr. Alon Retter>" <ar@astro.keele.ac.uk>
- Subject: [vsnet-chat 3934] Re: [vsnet-campaign-nova 123] Re: Possible Nova in Pup
- cc: vsnet-campaign-nova@kusastro.kyoto-u.ac.jp, vsnet-chat@kusastro.kyoto-u.ac.jp, vsnet-campaign-ip@kusastro.kyoto-u.ac.jp
- In-Reply-To: <200101021327.WAA08536@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
On Tue, 2 Jan 2001, Taichi Kato wrote:
> Re: Possible Nova in Pup
>
> > I saw soma mails with the new "nova" and have a question - is the
> > amplitude for the system common for novae? I suspect it quite small -
> > maybe reddening who knows but maybe southeners could perform some
> > high-speed photometry for oscilaltions...
>
> I think the possibility is very unlikely, as inferred from the
> progenitor color. High-speed photometry of this region of the sky should
> better be reserved for Alon Retter's TV Col campaign :-)
>
> Regards,
> Taichi Kato
Thank you for your support. I agree with you that fast photometry of
TV Col should be more valuable than observing the (unconfirmed) Nova
Pup 00. In addition, if the nova amplitude is indeed very small, then
its binary period is probably relatively long (say ~10 hours - a few
days). If the nova erupted last week, then it is probably too early to
reveal its orbital period.
I've nearly finished a night of continuous photometry on TV Col. So far
nearly 7 hours. I hope the weather continues to be so nice.
Best wishes,
Alon
-----------------------------------------------------------------------
Dr. Alon Retter Tel. (work) +44-(0)1782-58-3493
Physics Dept. Fax (work) +44-(0)1782-711093
Keele University -----------------------------------
Staffordshire, ST5 5BG 'As a scientist I don't believe myself, so
U.K. why should I believe you?' (A.R. 1965-2085)
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