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

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dc.creatorShears, Jeremy
dc.creatorPickard, Roger
dc.creatorKrajci, Tom
dc.creatorPoyner, Gary
dc.date2007-05-31
dc.date.accessioned2026-07-07T08:03:45Z
dc.date.available2026-07-07T08:03:45Z
dc.descriptionDuring 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.
dc.description10 pages, 9 figures. Accepted for publication in the Journal of the British Astronomical Association
dc.identifierhttps://arxiv.org/abs/0705.4611
dc.identifierhttp://arxiv.org/abs/0705.4611
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/129691
dc.subjectAstrophysics
dc.titlePhotometry of the dwarf nova AW Sagittae during the 2006 November superoutburst
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