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[vsnet-chat 3926] Possible Nova in Pup
- Date: Tue, 02 Jan 2001 14:39:19 +0200
- To: <tkato@kusastro.kyoto-u.ac.jp>, <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: "Berto Monard" <Lagmonar@csir.co.za>
- Subject: [vsnet-chat 3926] Possible Nova in Pup
- Disclaimer: The CSIR exercises no editorial control over E-mail messages originating in the organisation and the views in this message are therefore not necessarily those of the CSIR and/or its employees.
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Taichi, possibly the proper motion has a small radial component. Maybe the
object moves straight at us? Could it be the millenium X-mas star?
;--)
The photometric data so far (bright state for over a month) exclude a
typical CV outburst. Therefore I must agree that it is probably a nova but
possibly with a progenitor (around magn 21?) hidden behind the 14 th
magnitude star. This is a dense MW field.
In two months time we will know for sure.
Question No 1: Are there novae on record with a light gain of less
than 6 magnitudes? Subluminous types?
Question No 2: Is it possible that the 'nova' had been much brighter before
its discovery. Mr Haseda's photo precedes the actual discovery by nearly a
month. What happened the month before then (Oct 2000)? The region must have been
well above the horizon at that time. Bad weather?
Regards,
Berto
>>> Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> 01/02/01
01:40PM >>>
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.
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