Bolometric Correction of the roAp star $α$ Cir

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dc.creatorBrandão, I. M.
dc.creatorCunha, M. S.
dc.creatorGameiro, J. F.
dc.date2007-12-11
dc.date.accessioned2026-07-07T08:48:35Z
dc.date.available2026-07-07T08:48:35Z
dc.descriptionFor the first time, the bolometric correction of $α$ Cir was determined. Two values, both based on an estimation of the total integrated flux, were obtained. For that purpose spectroscopic and photometric data of $α$ Cir available in the literature was used. The values derived were then used to place $α$ Cir in the HR diagram.
dc.description2 pages, 1 figure, poster proceeding - Vienna, 2007 - CP/AP Workshop
dc.identifierhttps://arxiv.org/abs/0712.1697
dc.identifierhttp://arxiv.org/abs/0712.1697
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143993
dc.subjectAstrophysics
dc.titleBolometric Correction of the roAp star $α$ Cir
dc.typetext

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