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[vsnet-alert 744] CVC 129 (T Leo)
- Date: Fri, 21 Feb 1997 00:23:24 -0100
- To: tvanmuns@innet.be
- From: Tonny Vanmunster <tvanmuns@innet.be>
- Subject: [vsnet-alert 744] CVC 129 (T Leo)
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
BELGIAN ASTRONOMICAL SOCIETY V.V.S. - Working Group Variable Stars
Cataclysmic Variables Circular No.129 1997, February 20
Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM
Internet: tvanmuns@innet.be TEL. 32-11-831504
CBA Belgium Web Page : http://vsnet.astro.columbia.edu/~cba/be
===================================================================
T Leo [UGSU, 10B - 15.7B]
=========================
Robert Modic, USA has detected an outburst of T Leo, as announced
on vsnet. Following observations, confirming the outburst, have
been received so far :
1997 Feb 18.697 UT, <13.6 (Watanabe, VSOLJ, seq: GSC);
Feb 19.17 UT, <13.6 (P. Schmeer, Germany);
Feb 19.276 UT, 12.2 (R. Modic, USA);
Feb 19.347 UT, 11.9 (R. Modic);
Feb 19.489 UT, 10.9 (G. Hanson, USA);
Feb 19.500 UT, 10.9 (G. Hanson);
Feb 19.525 UT, 10.8 (G. Hanson);
Feb 19.533 UT, 10.4 (Watanabe);
Feb 19.549 UT, 10.7 (G. Hanson);
Feb 20.111 UT, 10.4 (Schmeer);
The previous outburst of T Leo was observed on 1995, November 13
by P. Schmeer [CVC 70], when the object reached mag. 10.4. It was
a poorly observed outburst [CVC 73].
T Leo is a remarkable object, in the sense that on a couple of
occasions, it has shown rebrightenings after outbursts (maybe
of a similar nature as the ones exhibited by GO Com, V1028 Cyg
and others). These secondary maxima of T Leo can be almost as bright
as the primary outburst, but last for only one day or so.
Since there is considerable interest in a detailed study of this
phenomenon, T Leo has been added to the CVAP programme in May 1995.
Our primary objective was to monitor a number of future outbursts
intensively in order to detect and follow-up these secondary
maxima [CVC 38].
We encourage our observers to continue monitoring this object
during its present outburst in the period after the initial decline.
With a little luck, the fading will occur without moonlight inter-
vening, hence providing an excellent opportunity to study T Leo,
which is now well placed in the evening sky.
Tonny Vanmunster
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