Curious Variables Experiment (CURVE). TT Bootis - superhump period change pattern confirmed

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dc.creatorOlech, A.
dc.creatorCook, L. M.
dc.creatorZloczewski, K.
dc.creatorMularczyk, K.
dc.creatorKedzierski, P.
dc.creatorUdalski, A.
dc.creatorWisniewski, M.
dc.date2004-08-04
dc.date.accessioned2026-07-07T02:14:13Z
dc.date.available2026-07-07T02:14:13Z
dc.descriptionWe report extensive multi-station photometry of TT Boo during its June 2004 superoutburst. The amplitude of the superoutburst was about 5.5 mag and its length over 22 days. The star showed a small re-brightening starting around the 9th day of the superoutburst. During entire bright state we observed clear superhumps with amplitudes from 0.07 to 0.26 mag and a mean period of Psh = 0.0779589(47) days (112.261 +/- 0.007 min). The period was not constant but decreased at the beginning and the end of superoutburst yet increased in the middle phase. We argue that the complicated shape of the O-C diagram is caused by real period changes rather than by phase shifts. Combining the data from two superoutbursts from 1989 and 2004 allowed us to trace the birth of the late superhumps and we conclude that it is a rather quick process lasting about one day.
dc.description14 pages, 6 figures, submitted to Acta Astronomica
dc.identifierhttps://arxiv.org/abs/astro-ph/0408080
dc.identifierhttp://arxiv.org/abs/astro-ph/0408080
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8029
dc.subjectAstrophysics
dc.titleCurious Variables Experiment (CURVE). TT Bootis - superhump period change pattern confirmed
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