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

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.

preprint2010arXivOpen access
S. Simón-DíazM. F. NievaN. PrzybillaG. Stasińska
astro-ph.SR
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Open access4 authors1 topic
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S. Simón-DíazM. F. NievaN. PrzybillaG. Stasińska

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