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[vsnet-chat 5124] Lambda Pavonis outburst
- Date: Mon, 25 Feb 2002 02:19:21 -0300
- To: "vsnet-chat" <vsnet-chat@kusastro.kyoto-u.ac.jp>, <vsnet-campaign-be@kusastro.kyoto-u.ac.jp>, <vsnet-be@kusastro.kyoto-u.ac.jp>, <vsnet-obs@kusastro.kyoto-u.ac.jp>
- From: "Sebastian Otero" <varsao@fullzero.com.ar>
- Subject: [vsnet-chat 5124] Lambda Pavonis outburst
- Cc: "Enzo M. De Bernardini" <enzodb@arnet.com.ar>, <surastronomico@yahoo.com>, "Lucho" <luchor@infovia.com.ar>, "paula Pietranera" <ppietranera@hotmail.com>, "T'Aanik.-" <taanik@yahoo.com.ar>
- Delivered-To: vsnet-chat@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
Dear all:
In our first observation of the year of lambda Pavonis, Cecilia Scalia and I
found the star in a extremely bright state: brighter than 4.0. We don't know
how long has been this bright state lasting. The GCVS lists the star as
varying between 4.00 and 4.26, but I noticed that in previous editions the
total range was as bright as 3.6. Maybe it was recorded but -given the
subsequent behaviour of the star- then rejected?
Anyway, keep an eye on it.
The normal quiescent state is around 4.15 - 4.27 in V.
PAVlambda 20020224.332 3.98 SCO
PAVlambda 20020224.334 3.98 OSE
Regards,
Sebastian and Cecilia.
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