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

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dc.creatorShears, Jeremy
dc.creatorBoyd, David
dc.date2006-08-03
dc.date.accessioned2026-07-07T07:19:17Z
dc.date.available2026-07-07T07:19:17Z
dc.descriptionWe 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.
dc.descriptionAccepted for publication in the Journal of the British Astronomical Association. 3 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0608082
dc.identifierhttp://arxiv.org/abs/astro-ph/0608082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/114571
dc.subjectAstrophysics
dc.titleDetermination of the superhump period of the dwarf nova V701 Tau during the 2005 December superoutburst
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