Massive stars vs. nebular abundances in the Orion nebula
Astrophysics
2007-05-23 v1
Abstract
The 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.
Cite
@article{arxiv.astro-ph/0611513,
title = {Massive stars vs. nebular abundances in the Orion nebula},
author = {Sergio Simón Díaz},
journal= {arXiv preprint arXiv:astro-ph/0611513},
year = {2007}
}
Comments
4 pages, 1 figure, to appear in "The Metal Rich Universe" Conference Proceedings