Properties of Regions Forming the FeII Emission Lines in Be Stars

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dc.creatorArias, Maria Laura
dc.creatorZorec, Juan
dc.creatorCidale, Lydia
dc.creatorRinguelet, Adela
dc.date2005-09-07
dc.date.accessioned2026-07-07T02:18:35Z
dc.date.available2026-07-07T02:18:35Z
dc.descriptionWe study FeII and Balmer hydrogen emission lines observed simultaneously of 18 southern Be stars. We use the self-absorption-curve method (SAC) to determine the optical depth regime of FeII emission lines and to derive first insights on the physical properties of their forming regions.
dc.descriptionSociete Francaise d'Astronomie et d'Astrophysique, France (2005)
dc.identifierhttps://arxiv.org/abs/astro-ph/0509178
dc.identifierhttp://arxiv.org/abs/astro-ph/0509178
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9544
dc.subjectAstrophysics
dc.titleProperties of Regions Forming the FeII Emission Lines in Be Stars
dc.typetext

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