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[vsnet-campaign 1223] RE: [vsnet-superoutburst 1171] 1RXS J232953.9+062814 outburst! (rebrightening?) - SUPEROUTBURSTING AGAIN
Dear colleagues,
A quick reply on Kato's message below (I have to leave the observatory for a
few hours now, a more detailed analysis will follow later today). The
rebrightening of 1RXS J232953.9+062814, that started on Nov 09/10, clearly
has developed into a superoutburst again, as I can derive from last night's
observations (Nov 10/11) at CBA Belgium Observatory. I was able to track the
object for 6.2 hours under perfect skies. The resulting light curve is truly
impressive, showing again 0.2 - 0.25 mag superhumps, superimposed by more or
less complex humps. Overall, there was also a definite fading trend.
I will further analyse the data, and distribute them later tonight. Please
continue monitoring this object !
Best regards,
Tonny Vanmunster
CBA Belgium Observatory
http://vsnet.lunarpages.com/cbabelgium
email : Tonny.Vanmunster@advalvas.be
> -----Original Message-----
> From: owner-vsnet-superoutburst@kusastro.kyoto-u.ac.jp
> [mailto:owner-vsnet-superoutburst@kusastro.kyoto-u.ac.jp]On Behalf Of
> Taichi Kato
> Sent: Sunday 11 November 2001 2:37 AM
> To: vsnet-alert@kusastro.kyoto-u.ac.jp;
> vsnet-campaign@kusastro.kyoto-u.ac.jp;
> vsnet-superoutburst@kusastro.kyoto-u.ac.jp
> Subject: [vsnet-superoutburst 1171] 1RXS J232953.9+062814 outburst!
> (rebrightening?)
>
>
> 1RXS J232953.9+062814 outburst! (rebrightening?)
>
> Dear Colleagues,
>
> We have received new data from Tonny Vanmunster, which clearly showed
> a rise toward a new maximum!! The maximum was also recorded by Maciej
> Reszelski on Nov. 9.758 UT at mag 13.0 (vsnet-obs 36808). We
> have receieved
> reports of successful observations last night (Nov. 10) at Bisei
> (Okayama),
> Miyazaki University (Miyazaki) (both relayed by K. Torii, RIKEN), and by
> T. Tanabe and K. Matsumoto (Okayama). All observations will be analyzed
> in due time. A quick look at Vanmunster's rising branch shows little
> evidence of superhumps, which might indicate that the present outburst
> is a normal-outburst type post-superoutburst rebrightening (a similar
> phenomenon was also recorded in V485 Cen) or a separate normal outburst.
>
> Intensive observations are most strongly requested to follow
> the evolution
> of the present outburst as densely as possible. Snapshot and
> time-resolved
> spectroscopy is also very encouraged.
>
> Further contact:
> photometry: M. Uemura (uemura@kusastro.kyoto-u.ac.jp)
> spectroscopy: R. Ishioka (ishioka@kusastro.kyoto-u.ac.jp)
>
> Regards,
> Taichi Kato
> on behalf of the VSNET Collaboration team
>
>
vsnet-adm@kusastro.kyoto-u.ac.jp
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