The chemical composition of the Orion star forming region: stars, gas and dust

Bibcode
2011BSRSL..80..255S
Simón-Díaz, S.; Nieva, M. F.; Przybilla, N.; Stasińska, G.
Bibliographical reference

Société Royale des Sciences de Liège, Bulletin, vol. 80, p. 255-259 (Proceedings of the 39th Liège Astrophysical Colloquium, held in Liège 12-16 July 2010, edited by G. Rauw, M. De Becker, Y. Nazé, J.-M. Vreux, P. Williams)

Advertised on:
1
2011
Number of authors
4
IAC number of authors
0
Citations
3
Refereed citations
3
Description
We present a summary of main results from the studies performed in the series of papers The chemical composition of the Orion star forming region. We reinvestigate the chemical composition of B-type stars in the Orion OB1 association by means of state-of-the-art stellar atmosphere codes, atomic models and techniques, and compare the resulting abundances with those obtained from the emission line spectra of the Orion nebula (M42), and recent determinations of the Solar chemical composition.
Type
Non-refereed

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