Hydrogen neutral outflowing disks of B[e] supergiants

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dc.creatorKraus, M.
dc.creatorFernandes, M. Borges
dc.creatorde Araujo, F. X.
dc.date2007-02-14
dc.date.accessioned2026-07-07T07:46:45Z
dc.date.available2026-07-07T07:46:45Z
dc.descriptionThe [O I] line emission of the LMC B[e] supergiant R126 is modeled with an outflowing disk scenario. We find that hydrogen in the disk must be ionized by less than 0.1%, meaning that the disk material is predominantly neutral. The free-free emission is calculated from the polar wind, and the minimum density contrast between disk and polar wind is found to be ~10.
dc.description2 pages, to appear in Rev. Mex. Astron. Astrof. Conf. Ser., ed. P. Benaglia, G. Bosch and C.E. Cappa, Proceedings of the workshop on Massive Stars held in Carilo, Argentina, Dec. 11-14, 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0702372
dc.identifierhttp://arxiv.org/abs/astro-ph/0702372
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/123932
dc.subjectAstrophysics
dc.titleHydrogen neutral outflowing disks of B[e] supergiants
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