Fast Rotation vs. Metallicity

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dc.creatorLevenhagen, Ronaldo
dc.creatorLeister, Nelson Vani
dc.creatorZorec, Juan
dc.creatorFremat, Yves
dc.date2005-09-07
dc.date.accessioned2026-07-07T02:18:36Z
dc.date.available2026-07-07T02:18:36Z
dc.descriptionFast rotation seems to be the major factor to trigger the Be phenomenon. Surface fast rotation can be favored by initial formation conditions such as metal abundance. Models of fast rotating atmospheres and evolutionary tracks are used to determine the stellar fundamental parameters of 120 Be stars situated in spatially well-separated regions to imply there is between them some gradient of metallicity. We study the effects of the incidence of this gradient on the nature of the studied stars as fast rotators.
dc.descriptionSociete Francaise d'Astronomie et d'Astrophysique, France (2005)
dc.identifierhttps://arxiv.org/abs/astro-ph/0509179
dc.identifierhttp://arxiv.org/abs/astro-ph/0509179
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9545
dc.subjectAstrophysics
dc.titleFast Rotation vs. Metallicity
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