Massive stars vs. nebular abundances in the Orion nebula

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dc.creatorDíaz, Sergio Simón
dc.date2006-11-16
dc.date.accessioned2026-07-07T07:30:51Z
dc.date.available2026-07-07T07:30:51Z
dc.descriptionThe search of consistency between nebular and massive star abundances has been a longstanding problem. I briefly review what has been done regarding to this topic, also presenting a recent study focused on the Orion nebula: the O and Si stellar abundances resulting from a detailed and fully consistent spectroscopic analysis of the group of B stars associated with the Orion nebula are compared with the most recent nebular gas-phase results.
dc.description4 pages, 1 figure, to appear in "The Metal Rich Universe" Conference Proceedings
dc.identifierhttps://arxiv.org/abs/astro-ph/0611513
dc.identifierhttp://arxiv.org/abs/astro-ph/0611513
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/118544
dc.subjectAstrophysics
dc.titleMassive stars vs. nebular abundances in the Orion nebula
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