Rapid Variations in V2275 Cyg (Nova Cyg 2001 #2)

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dc.creatorGarnavich, P. M.
dc.creatorMacdonald, A. J.
dc.creatorWu, B.
dc.creatorEasterday, S. M.
dc.creatorLibal, A. J.
dc.creatorPalumbo, A.
dc.creatorQuinn, M. A.
dc.date2004-01-11
dc.date.accessioned2026-07-07T02:11:50Z
dc.date.available2026-07-07T02:11:50Z
dc.descriptionWe present time-resolved CCD photometry of V2275 Cyg 790 days after the nova outburst. The data show a 20% peak-to-peak oscillation with a period of 24 minutes. The period appears stable over the two nights of observation, but QPO can not be ruled out.
dc.description3 pages, 3 postscript figures, uses ibvs2.sty, to be published in IBVS
dc.identifierhttps://arxiv.org/abs/astro-ph/0401183
dc.identifierhttp://arxiv.org/abs/astro-ph/0401183
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7246
dc.subjectAstrophysics
dc.titleRapid Variations in V2275 Cyg (Nova Cyg 2001 #2)
dc.typetext

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