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[vsnet-j 1752] HT Cam: very strong modulation!!
- Date: Mon, 31 Dec 2001 14:05:41 +0900 (JST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign-dn@kusastro.kyoto-u.ac.jp, vsnet-campaign-ip@kusastro.kyoto-u.ac.jp, vsnet-ip@kusastro.kyoto-u.ac.jp, vsnet-outburst@kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-j 1752] HT Cam: very strong modulation!!
- Cc: vsnet-j@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-j@ooruri.kusastro.kyoto-u.ac.jp
HT Cam: very strong modulation!!
Dear Colleagues,
We have partly analyzed the Kyoto and RIKEN (Torii-san) data.
The initial result is surprizing.
Superimposed on the decay, as inferred from visual and other observations,
there exist *very strong* (0.4 mag or even larger) short-term modulations.
Although exact identification requires further analysis (of the full-night
data) and period analysis, the modulations seem to be somehow related to
the 8.5-min period reported by Tovmassian. This finding may be indicative
of the (possibly transient) IP (intermediate polar) nature of this object.
[Note, however, optical photometry during an outburst of DO Dra, did show
a similar (lower amplitude) periodicity which does not agree with the
spin period].
The large-amplitude short-term modulations are quite unlike any modulations
seen during an outburst of any CV. The characteristics are even drastically
different from that reportd by Gary W. Billings (vsnet-alert 6953)
less than 0.5 d ago! Observers are strongly requested to continue
observing this object as intensively as possible, since we may have
witnessed a short period of unexpectedly intensive avtivity of this CV.
Regards,
Taichi Kato
VSNET Collaboration team