[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-obs 774] CVC 46 (V542 Cyg)
- Date: Mon, 17 Jul 1995 02:13:34 +0200
- To: observations@aavso.org, j.bortle@genie.geis.com, guy@tahq.demon.co.uk, tkato@kusastro.kyoto-u.ac.jp, gp@star.sr.bham.ac.uk, pvancaut@innet.be, bill.worraker@aea.orgn.uk, nogami@kusastro.kyoto-u.ac.jp, extpasc@rz.uni-sb.de, steyaert@vvs.innet.be, 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@fid.planet.zpok.hu
- From: tvanmuns@innet.be (Tonny Vanmunster)
- Subject: [vsnet-obs 774] CVC 46 (V542 Cyg)
- Reply-To: vsnet-obs@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
BELGIAN ASTRONOMICAL SOCIETY V.V.S. - Working Group Variable Stars
Cataclysmic Variables Circular No.46 1995, July 17
Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM
Internet: tvanmuns@innet.be TEL. 32-11-831504
P. Van Cauteren, de Borrekenslaan 54, 2630 Aartselaar, BELGIUM
Internet: pvancaut@innet.be TEL. 32-3-8774098
===================================================================
V542 Cyg [UGSS:, 13.0p - 18.3:p]
================================
Tonny Vanmunster, Landen, Belgium reports an outburst detection of
V542 Cyg, which is on the Recurrent Objects Programme of TA/BAAVSS.
Confirmation has come from Eric Broens, Mol, Belgium. CVC 23 briefly
discusses remarks on the classification of V542 Cyg as a dwarf nova.
1995 Jul 10.053 UT, [13.9 (T. Vanmunster, 0.35-m refl., seq: AAVSO);
Jul 13.906 UT, [13.5 (T. Vanmunster, strong moonlight);
Jul 14.955 UT, 13.8 (T. Vanmunster, moonlight);
Jul 15.997 UT, 13.9 (T. Vanmunster);
Jul 16.894 UT, 13.9 (T. Vanmunster);
Jul 16.945 UT, 13.7 (E. Broens, 0.35-m refl., seq: AAVSO);
V542 Cyg was last reported in outburst on December 21, 1994 by Gary
Poyner, UK [CVC 23] and reached maximum brightness (mag. 13.4) the
day after. The outburst lasted for more than 10 days [CVC 25].
A photometric summary, covering a much brighter outburst of V542 Cyg
in June 1994, which lasted approximately 12 days, is given in CVC 9.
BC UMa [UGSU, 10.9B - 18.3B]
============================
The BC UMa outburst, reported in CVC 45, apparently was a normal
outburst, as communicated by Janet Mattei, AAVSO : "The following
observations [completed with other ones submitted over VSNET - Ed.]
indicate that the recent outburst of BC UMa has ended. This outburst
was a short one, lasting a little more than 2 days.
BC UMA 950702.965 UT <14.0 G. Poyner, BAA,AAVSO
950705.8 <14.0 L. Szentasko, VSNET
950706.1576 14.0 D. York, AAVSO
950706.1694 13.9 York
950706.1868 13.8 York
950706.2076 13.4 York
950706.2292 13.0 York
950706.8576 13.0 Szentasko
950707.10 12.4 G. Dyck, AAVSO
950707.1542 13.2 York
950707.1708 13.2 York
950707.2347 13.0 T. Burrows, AAVSO
950707.86 14.2 Szentasko
950708.23 <13.6 Burrows
950708.24 <13.6 Burrows
950708.25 <13.6 Burrows
950708.86 15.1 Szentasko
950708.89 <13.6 J. Gunther, AFOEV, AAVSO (via VSNET)
950710.2535 <15.5 R. Royer, AAVSO
All observations were made using the AAVSO sequence."
Janet Mattei further adds : "BC UMa has been closely monitored by the AAVSO
since 1971. Observations in the AAVSO International Database indicate that
BC UMa has had only the following four long outbursts (superoutbursts?)
since 1971: May 1982, September 1990, August 1992, and April 1994, each
lasting between 7 to 9 days. In addition, there are several unconfirmed,
single observations, in the BC UMa data files. From the short duration of
the recent well-monitored outburst, there is a possibility that some of the
short outbursts may have been missed, and that the single, positive
observations may be part of short outbursts."
Tonny Vanmunster