Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-05-18
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
18 pages, 4 figures. Accepted for publication in JBAA
Scientific paper
We report the discovery of a new dwarf nova and our observations of its first confirmed superoutburst during 2009 October. The outburst amplitude was 6 magnitudes. The main outburst lasted 17 days and was followed 4 days later by a remarkable rebrightening. Superhumps were present during the main outburst, which confirms that it belongs to the SU UMa family. Initially the mean superhump period was Psh = 0.06965(17) d, but analysis of the O-C residuals showed a dramatic evolution in Psh during the outburst. During the first two-thirds of the plateau phase the period increased with dPsh/dt = +1.24(5) x 10-3. There was then an abrupt change following which the period decreased with dPsh/dt = -1.01(9) x 10-3. The amplitude of the superhumps also varied, with a maximum amplitude near the beginning of the outburst and a second maximum corresponding to the discontinuity in Psh. Analysis of archival data showed outbursts also occurred in October 2005, June 2006 and June 2007. Assuming that the superoutbursts are periodic, we estimate that the outburst period is around 450 days.
Bolt G. G.
Hambsch Franz-Josef
Krajci Tom
Miller Ian
Sabo Richard
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