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[vsnet-alert 1448] CVC 161 [SBS 1017+533 new UGSU star]
- Date: Sun, 1 Feb 1998 15:13:23 +0100 (MET)
- To: tvanmuns@innet.be
- From: Tonny Vanmunster <tvanmuns@innet.be>
- Subject: [vsnet-alert 1448] CVC 161 [SBS 1017+533 new UGSU star]
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
BELGIAN ASTRONOMICAL SOCIETY V.V.S. - Working Group Variable Stars
Cataclysmic Variables Circular No.161 1998, February 01
Ed.: T. Vanmunster, Walhostraat 1A, 3401 Landen, BELGIUM
Internet: tvanmuns@innet.be TEL. 32-11-831504
CVC Web Page : http://vsnet.astro.columbia.edu/~cba/cvc
===================================================================
SBS 1017+533 [UGSU, 13? - 16?]
==============================
Peter Garnavich recently reported his detection of an outburst of
SBS 1017+533 [VSNET alert 1441]. He also reported spectral observations,
showing broad Balmer absorption lines, but weak Halpha emission.
Unfiltered CCD photometry by Tonny Vanmunster, CBA Belgium Observatory,
on 1998, January 31, using a 0.25-m telescope and ST-7 CCD camera,
reveals the existence of a periodic modulation in this system, which
has the typical signature of a superhump. It therefore is most likely
that SBS 1017+533 is a new member of the SU UMa-type cataclysmic
variables !
Our observations were made under quite unfavourable conditions (strong
windws), during a 7.8h observing session and show a periodic signal
at 0.069 +/- 0.001 d, with a mean semi-amplitude of 0.11 mag, after
heliocentric correction and removal of a linear trend of decline
(period determined using the PDM method).
SBS 1017+533 is located at RA = 10h20m26.65s and decl = +53d04'32.6"
(Epoch J2000.0).
Follow-up time-series CCD photometry is highly recommended.
Editorial Absence
-----------------
Please note that the Editor will be absent in the period from
February 9th till February 17th, 1998.
Tonny Vanmunster
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