Photometry of the dwarf nova AW Sagittae during the 2006 November superoutburst

Details Photometry of the dwarf nova AW Sagittae during the 2006 November superoutburst Photometry of the dwarf nova AW Sagittae during the 2006 November superoutburst

2007-05-31

arxiv.org/abs/0705.4611v1

Astronomy and Astrophysics

Astrophysics

10 pages, 9 figures. Accepted for publication in the Journal of the British Astronomical Association

Scientific paper

During 2006 November an outburst of the dwarf nova AW Sge was observed using CCD photometry. This revealed 0.25 magnitude superhumps confirming it to be a superoutburst, possibly only the second confirmed such outburst of this star. The superhumps were observed for 4 days and had a stable period Psh = 0.0745(2)d, a value which is consistent with Psh measured during the 2000 superoutburst.

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