Superhumps in V1141 Aquilae

dc.creatorOlech, A.
dc.date2003-02-19
dc.date.accessioned2026-07-07T02:07:39Z
dc.date.available2026-07-07T02:07:39Z
dc.descriptionThe results of the CCD observations of the 2002 superoutburst of V1141 Aql are described. We have detected clear superhumps characterized by the period of 0.05930(5) days. There was another, much weaker, modulation in the light curve of V1141 Aql. Its amplitude is equal to $0.012\pm0.002$ mag and its period to 0.03923(8) days. We have also discovered quasi periodic oscillations (QPOs) with a mean period equal to 130 s and amplitude of $0.025\pm0.004$ mag.
dc.descriptionsubmitted to Acta Astronomica, 11 pages, 8 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0302379
dc.identifierhttp://arxiv.org/abs/astro-ph/0302379
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5766
dc.subjectAstrophysics
dc.titleSuperhumps in V1141 Aquilae
dc.typetext

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