Bulletin de la Société Royale des Sciences de Liège

0037-9565 1783-5720

 

sinds 05 februari 2011 :
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S. Simón-Díaz, M. F. Nieva, N. Przybilla & G. Stasínska

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

(Volume 80 - Année 2011)
Article
Open Access

Abstract

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.

Om dit artikel te citeren:

S. Simón-Díaz, M. F. Nieva, N. Przybilla & G. Stasínska, «The chemical composition of the Orion star forming region: stars, gas and dust», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 80 - Année 2011, 255 - 259 URL : http://popups.ulg.be/0037-9565/index.php?id=2729.

Over : S. Simón-Díaz

Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain, and Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain

Over : M. F. Nieva

Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany

Over : N. Przybilla

Dr. Karl Remeis-Sternwarte & ECAP, Sternwartstr.7, D-96049 Bamberg, Germany

Over : G. Stasínska

LUTH, Observatoire de Paris, CNRS, Université Paris Diderot, F-92190 Meudon, France