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[vsnet-chat 3922] [vsnet-alert 5499] Re: Possible Nova in Pup
- Date: Tue, 02 Jan 2001 12:09:57 +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 3922] [vsnet-alert 5499] Re: 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
Dear Taichi and nova enthousiasts,
If the located star is indeed the progenitor of the brightened object then
its presumed nova nature is improbable.
I still believe (and might have mentioned it earlier) that the Pup-Pyx-Vel
region must be one of the most under explored MW region in the sky and quite a
number of CVs might still be discovered there. This Nova? Pup 00 might be one of
them...
Regards,
Berto
PS I didn't read e-mail since 24/12/00 and found quite some interesting
findings in my e-box. VSNET is doing a great info job!
We have to keep watch on TV Col. Could it be in a transition stage?
This is an exciting hobby!
>>> Taichi Kato
<tkato@kusastro.kyoto-u.ac.jp> 01/02/01 11:59AM >>>
Re:
Possible Nova in Pup
> I'm not able to identify this star on USNO A2.0
(no entry like this around
> the suspetc position). As I said earlier, a
good USNO A2.0 progenitor
> candidate (if this actually is a nova) is
A0600.06937901; is, the entry
> above, related to a different USNO
catalogue (A1.0, SA, AC2000...)? Please
> note also that there is some
difference in coordinates between A0600.06937901
> (which I indicate to be
the probable progenitor) and USNO0600.03989187. So,
> it could be
interesting to know if the star reported by Dr. Kato comes from
> a
different USNO catalogue. Maybe these stars are the same.
These stars are the same. I used USNO A1.0. If we adopt the USNO
A2.0
magnitudes, the V-J color is even more bluer (closer to a slightly
reddened
cataclysmic variable). I wonder how accurate A2.0 photometric
calibration
in this field.
Regards,
Taichi Kato
PS. If this
object is indeed a nova (I suspect so...), the proginitor
is
one of the brightest ones in the recent
dacades.
Return to Daisaku Nogami
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