Rotation of 10 Be stars through Fourier transform analysis

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dc.creatorGavrilovic, Natasa
dc.date2006-02-28
dc.date.accessioned2026-07-07T07:00:54Z
dc.date.available2026-07-07T07:00:54Z
dc.descriptionHere we determine the projected rotational velocity of 10 Be stars using Fourier Transform Method. Also, we discuss the gravity darkening and extend of deviation from solid body rotation for our sample of stars. We found that 7 of considered stars are affected by strong gravity darkening or/and solar differential rotation.
dc.description3 pages, 1 figure, 1 table, accepted in Publ. Obs. Astron. Belgrade No. 80
dc.identifierhttps://arxiv.org/abs/astro-ph/0602620
dc.identifierhttp://arxiv.org/abs/astro-ph/0602620
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/108122
dc.subjectAstrophysics
dc.titleRotation of 10 Be stars through Fourier transform analysis
dc.typetext

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