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[vsnet-chat 3927] Re: Possible Nova in Pup
- Date: Tue, 02 Jan 2001 13:46:59 +0100
- To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Rudolf Novak <novak@hvezdarna.cz>
- Subject: [vsnet-chat 3927] Re: Possible Nova in Pup
- Organization: Nicholas Copernicus Observatory in Brno
- References: <200101021140.UAA00947@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
- User-Agent: Mozilla/5.0 (X11; U; Linux 2.2.16-22 i586; en-US; 0.6) Gecko/20001205
Dear dr. Kato,
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...
Rudolf Novak
Taichi Kato wrote:
> Re: [vsnet-chat 3924] Possible Nova in Pup
>
>> UGWZ type CV like RZ Leo perhaps?
>> A not too far away system, with a small reddish secondary, low accretion
>> rate, undetected so far but with the bluish colour of the hot WD...
>>
>> Is this not a nearby part of the Milky Way?
>
>
> If it were so, we should have selected it as the top-priority photometric
> campaign target :-)
>
> I don't think it a very nearby object, considering the undetectable
> proper motion between the POSS and present epochs.
>
> Regards,
> Taichi Kato
>
>
>
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