SDSSp J173008.38+624754.7: Very Short Supercycle

As reported by M. Simonsen on February 18, the SU UMa-type dwarf nova SDSSp J173008.38+624754.7 experienced a bright (13.6mag) outburst (vsnet-campaign-dn 2131). The Kyoto team performed time-series photometry on February 20 (vsnet-campaign-dn 2138), and detected superhumps with amplitude of 0.3mag (vsnet-campaign-dn 2140). This outburst was thus a superoutburst, and the supercycle of the object is around 100 d, which is one of the shortest supercycles in usual SU UMa-type dwarf novae (vsnet-campaign-dn 2131). The Kyoto team reported that the object faded at a rate of ~0.3 mag/day on February 20-22. The combined light curve showed a period of 0.073557(44) d (vsnet-campaign-dn 2143).

Another superoutburst (13.9mag) was reported by M. Simonsen on September 10 (vsnet-campaign-dn 2821). The outburst was confirmed by A. Oksanen at about 13.7mag (vsnet-campaign-dn 2828, 2829, 2873).

An outburst (14.7mag) was reported by T. Kinnunen on December 23.  A fading to 15.3: mag was reported on December 24.  It may be a normal outburst (vsnet-campaign-dn 3191).

Other articles:
vsnet-campaign-dn 2134, 2832, 2842, 2852

Links:

Chart with CCD(V) sequences:
http://joevp.20m.com/charts/sloan/charts/
[vsnet-campaign-dn 2132]

CCD image during the October 2001 outburst by A. Oksanen:
 http://www.jklsirius.fi/obs/sdss1730map.jpg
[vsnet-campaign-dn 2133]

Light curve observed by A. Oksanen:
 http://nyrola.jklsirius.fi/ccd/2002/data0911/SDSS173020020911.jpg
 [vsnet-campaign-dn 2846]

General Information about This Object





Return to HomePage

Return to Daisaku Nogami's page


vsnet-adm@kusastro.kyoto-u.ac.jp

Powered by ooruri technology