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[vsnet-alert 7205] Nova V1039 Cen 2001 - possible periodicity
- Date: Fri, 22 Feb 2002 11:02:44 +1100 (EST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign-nova@kusastro.kyoto-u.ac.jp
- From: Alon Retter <retter@Physics.usyd.edu.au>
- Subject: [vsnet-alert 7205] Nova V1039 Cen 2001 - possible periodicity
- Cc: Marc Bos <molehill@ihug.co.nz>, Sumner Starrfield <sumner.starrfield@asu.edu>, Berto Monard <Lagmonar@csir.co.za>, Peter Nelson <pnelson@dcsi.net.au>
- Delivered-To: vsnet-alert@kusastro.kyoto-u.ac.jp
- Reply-To: Alon Retter <retter@Physics.usyd.edu.au>
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
Dear southern vsneters,
Continuous CCD photometry carried out by Marc Bos (Mt Molehill
Observatory) during 5 hours on Monday (18/2/2) with no filter
shows nearly 3 cycles of a ~1.7-h modulation with a full amplitude
of ~0.05 mag. More observations are strongly encouraged to confirm
the presence of the possible periodicity. There are a few other
weak signals at higher frequencies but below the detection limit.
This result may be very significant.
If confirmed, the 1.7-h period can have 3 simple interpretations:
1. Orbital period (however, there are only 3-4 known novae with
orbital periods below the period gap (below ~2 h), so it is
quite interesting. In comparison, there are ~50 novae with
orbital periods > 3 h.
2. Superhump period (positive or negative superhump). In this case
the orbital period, would be very close to ~1.7 h (a few percent
shorter/longer). More data may show 1-2 more periods (the
orbital period and the other type of superhump).
3. Spin period. According to my untrustable memory the longest spin
period known in intermediate polars is ~1.1 h, although there are
two candidates with longer periods (~1.5 h, ~2 h). So, V1039 Cen
is at the top of this range. In this case, another longer period
(the orbital period) may be discovered with more data. I expect a
period of ~5-7 h in this case. Other periods, which result from
various combinations of the two periods may be discovered as well.
There are actually a few other possibilities with lower chances, that
I prefer not to mention here.
Option 3 would probably support my suggestion for a correlation between
the transition phase in novae and intermediate polars as V1039 Cen seem
to have had a few long-term oscillations with full amplitude of ~1 mag.
Options 1+2 still don't kill this idea as spin periods are best seen in
the X-Ray, not the optical. Thus, we need an X-Ray run - probably with
Chandra. Your result will sure help writing the proposal in plan.
Regards,
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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