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[vsnet-obs 2430] CVC 88 (SX LMi)
- Date: Wed, 20 Mar 1996 21:48:35 -0100
- To: observations@aavso.org, JBortle@AOL.com, guy@tahq.demon.co.uk, tkato@kusastro.kyoto-u.ac.jp, gp@star.sr.bham.ac.uk, lasse.teist@thranethrane.dk400.dk, pvancaut@innet.be, bill.worraker@aea.orgn.uk, nogami@kusastro.kyoto-u.ac.jp, safnet@mesiob.obspm.fr, KFA02524@niftyserve.or.jp, sno@iris.elte.hu, vsnet-obs@kusastro.kyoto-u.ac.jp, NAH01147@niftyserve.or.jp, ebroens@innet.be, fidusz@alba.zpok.hu
- From: Tonny Vanmunster <tvanmuns@innet.be>
- Subject: [vsnet-obs 2430] CVC 88 (SX LMi)
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
BELGIAN ASTRONOMICAL SOCIETY V.V.S. - Working Group Variable Stars
Cataclysmic Variables Circular No.88 1996, March 20
Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM
Internet: tvanmuns@innet.be TEL. 32-11-831504
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The CATACLYSMIC VARIABLES Home Page: http://vsnet.cv.psi.edu
===================================================================
SX LMi [UGSU, 13 - 17.4V]
=========================
We have received confirmative observations for the SX LMi outburst,
announced in our previous Circular. Rudolf Novak, Brno, Czech Republic
has forwarded us CCD observations, which he obtained on March 20,
1996, using an ST-7 CCD with R-filter, at the Ondrejov Observatory.
Comparison star was the object labeled [1219(1207)] on the chart
published in the Cataclysmic Variables Home Page. Magnitudes presented
below are provisional only and need further calibration.
1996 Mar 15.828 UT, [14.5 (T. Vanmunster, 0.35-m refl., seq: GSC);
Mar 18.853 UT, 13.5 (L. Jensen, Denmark);
Mar 19.820 UT, 13.5 (L. Jensen);
Mar 20.052 UT, 14.6 (R. Novak, Czech Republic, CCD R-filter);
Mar 20.056 UT, 14.8 (R. Novak);
Mar 20.060 UT, 14.7 (R. Novak);
Mar 20.067 UT, 14.7 (R. Novak);
Mar 20.071 UT, 14.7 (R. Novak);
Mar 20.074 UT, 14.8 (R. Novak);
Mar 20.078 UT, 14.8 (R. Novak);
Mar 20.079 UT, 14.8 (R. Novak);
Mar 20.081 UT, 14.9 (R. Novak);
Mar 20.084 UT, 14.6 (R. Novak);
Mar 20.085 UT, 14.7 (R. Novak);
Tonny Vanmunster