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[vsnet-chat 1600] Re: [vsnet-alert 2575] Nova Mus 98 - a possible periodicity
- Date: Tue, 2 Feb 1999 19:10:09 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 1600] Re: [vsnet-alert 2575] Nova Mus 98 - a possible periodicity
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: [vsnet-alert 2575] Nova Mus 98 - a possible periodicity
Dear Dr. Retter,
> Yes, this is certainly a possibility. The large outburst amplitude and the
> presence of the possible period might be explained by a magnetic nova
> model, as well.
Yes, it's another fascinating possibility. As may be remembered, at least
one magnetic nova (V1500 Cyg) indeed exists, and showed large-amplitude
variation which has been interpreted as the "search-light" phenomenon.
It would be interesting to search for this possibility in Nova Mus 1998, too.
As a matter of fact, my time-series pghotometry on Nova Her 1991 (V838 Her)
was motivated by the hope of detecting similar modulations.
> An intriguing suggestion is that the oscillations observed during
> the transition phase are caused by the reformation of the accretion disc.
> Anyway, this question is still opened.
I tend to think these oscillation as some kind of pulsation (or
instability) in the expanding shell (wind). I obtained some intermediate
band photometry in Nova Cas 1993 (V705 Cas), which showed ~2-day oscillation,
and found color changes and light curve profile similar to those of
pulsating variable. But it would be still premature to conclude anything
from this finding. I hope someone in the southern hemisphere follow the
oscillation cycle by multicolor photometry, and possibly by spectroscopy
to search for a signature of pulsation.
Regards,
Taichi Kato
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