Photometry of the dwarf nova AW Sagittae during the 2006 November superoutburst
classification
🌌 astro-ph
keywords
duringsuperoutburstdwarfnovanovemberobservedoutburstphotometry
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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.
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