2007/05/31 by Shears, Jeremy, Pickard, Roger, Krajci, Tom +1
#Astrophysics (astro-ph) #FOS: Physical sciences
paper · doi:10.48550/arxiv.0705.4611
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.