The chemical composition of the Orion star forming region: stars, gas and dust - Archive ouverte HAL
Article Dans Une Revue Bulletin de la Société Royale des Sciences de Liège Année : 2011

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

Résumé

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.

Dates et versions

hal-03796989 , version 1 (04-10-2022)

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S. Simón-Díaz, M. F. Nieva, Norbert Przybilla, Grazyna Stasinska. The chemical composition of the Orion star forming region: stars, gas and dust. Bulletin de la Société Royale des Sciences de Liège, 2011, 80, pp.255-259. ⟨hal-03796989⟩
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