On the Amplitudes of Superhumps

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dc.creatorSmak, J.
dc.date2009-01-16
dc.date.accessioned2026-07-07T13:03:35Z
dc.date.available2026-07-07T13:03:35Z
dc.descriptionAmplitudes of bolometric light curves produced by 2D and 3D simulations are used to determine the corresponding visual amplitudes. They turn out to be about 10 times lower than typical amplitudes of superhumps. This means a major failure of the tidal model of superhumps.
dc.description5 pages, submitted to "Acta Astronomica"
dc.identifierhttps://arxiv.org/abs/0901.2420
dc.identifierhttp://arxiv.org/abs/0901.2420
dc.identifierActa Astron., 59,103,2009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/226854
dc.subjectSolar and Stellar Astrophysics
dc.titleOn the Amplitudes of Superhumps
dc.typetext

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