[vsnet-alert 6384] Re: [vsnet-superoutburst 723] WZ Sge: rebrightening, more analysis

["Stan Walker" <astroman@voyager.co.nz>]

Greetings,

Well, at Aug 20.3 to 20.5 the star seemed to be varying between 13.1 and
13.6 based on Arne's values for the close companion star. The mean value
might have faded a few percent over that interval. But the eclipses and
superhumps looked good.

Regards,
Stan

----- Original Message -----
From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
To: <vsnet-alert@kusastro.kyoto-u.ac.jp>;
<vsnet-campaign-dn@kusastro.kyoto-u.ac.jp>;
<vsnet-superoutburst@kusastro.kyoto-u.ac.jp>
Sent: Tuesday, August 21, 2001 2:22 PM
Subject: [vsnet-superoutburst 723] WZ Sge: rebrightening, more analysis


> WZ Sge: rebrightening, more analysis
>
> Dear Colleagues,
>
>     We have received additional high-quaility data from B. Martin.
> Combined with the previous data, and the new analysis of Kyoto data,
> there seems to have been a minimum of brightness in early Aug. 20 (UT).
> The object has a more rapid brightening trend during the latter half
> of Aug. 20.  This may be an indication of an immediate full rebrightening.
> Please keep the closest watch!!
>
>     The profiles of eclipses vary, but the sharp, deep eclipses are
> present throughout this brightening phase.
>
>     More detailed analysis, and Web update, will be presented later
> by Uemura-san.
>
> Regards,
> Taichi Kato
> VSNET Collaboration team
>
>

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