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

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

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/129691

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0705.4611
 http://arxiv.org/abs/0705.4611

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arXiv