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Determination of the superhump period of the dwarf nova V701 Tau during the 2005 December superoutburst

Jeremy Shears·David Boyd
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Abstract

We report new measurements of the superhump period of the UGSU-type dwarf nova V701 Tau during the 2005 December superoutburst. Using unfiltered time series CCD observations on 3 nights, we determine a probable superhump period Psh = 0.0690, plus or minus 0.0002d, but note that our data also permit a possible shorter period of 0.0663, plus or minus 0.0002d. The longer period agrees with the value measured during the first recorded superoutburst in 1995.

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Jeremy Shears, David Boyd. 2006-08-03. Determination of the superhump period of the dwarf nova V701 Tau during the 2005 December superoutburst. https://arxiv.org/abs/astro-ph/0608082

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