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[vsnet-alert 4978] V1494 Aql - a photometric period of 1.5 hr - ?
- Date: Wed, 14 Jun 2000 14:23:35 +0100 (BST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Alon Retter <ar@astro.keele.ac.uk>
- Subject: [vsnet-alert 4978] V1494 Aql - a photometric period of 1.5 hr - ?
- cc: Tim Naylor <timn@astro.keele.ac.uk>, Nye Evans <ae@astro.keele.ac.uk>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear vsneters,
CCD photometry of V1494 Aql (Nova Aql 1999 No. 2) during 3 nights
in 2000 June through an R-band filter with the 0.4-m telescope at
N. Copernicus Observatory (Brno, Czech republic) reveals evidence
for a periodicity of 1.5 hours. The peak-to-trough amplitude of the
variation is about 0.05 mag. Continuous photometry is thus highly
recommended to confirm this period and to find out its nature. Red
filters are preferred, but other bands are fine.
Cor. of the nova (J2000.0):
19h 23m 05s.38
+04o 57' 20".1
V magnitude: mV~10.3
Why is it important:
1. The nova is very bright now. When the nova fades it will
be much harder to confirm the presence of the periodicity.
2. Observing the nova at this stage should teach us about the
evolution of the accretion activity in the nova at this stage
and onwards.
3. If the 1.5-h is the orbital period of the nova, it will be the 4th
confirmed nova below the period gap. Novae with periods below the
gap are important since Retter & Naylor (2000) suggested that
post-novae below the gap don't return fast to their pre-outburst
magnitudes as novae above the gap do. This might be the first evidence
for mass transfer cycles in CVs.
4. If the period is a superhump period, then the orbital period will be
very similar, and the conclusions of section 3. stay the same.
5. If the 1.5-h is the spin period of the nova, and the orbital period
will be longer, then the nova should be an intermediate polar.
V1494 Aql had oscillations during its transition phase. Thus this
would confirm Retter, Liller and Gerrard (1999) suggestion of a link
between intermediate polars and the oscillations / dust during the
transition phase in classical novae.
Regards,
Alon
-------------------------------------------------------------------------
Dr. Alon Retter Tl. (work) +44-(0)1782-58-3493
Physics Dept. Fax (work) +44-(0)1782-711093
Keele University -----------------------------------
Staffordshire 'As a scientist I don't believe myself, so
ST5 5BG, U.K. why should I believe you?' (A.R. 1965-2085)
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