Add to ORKGInternational audienceWe 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
Context. Modern spectroscopy of early-type stars often aims at studying complex physical phenomena ...
Due to its proximity, the Orion star forming region is often used as a proxy to study processes rela...
Abstract. This review discusses recent results on the astrochemistry of (mostly high-mass) star-form...
International audienceWe present a summary of main results from the studies performed in the series ...
Context. Early B-type stars are invaluable indicators of elemental abundances of their bir...
Context. Recent accurate abundance analyses of B-type main sequence stars in the solar vicinity has...
International audience Aims: We re-examine the recombination/collisional emission line (RL/CEL) nebu...
We present non-LTE oxygen abundances for a sample of B stars in the Orion association. The abundance...
Context. The evolution of chemical elements in a galaxy is linked to its star formation history. Var...
As one of the nearest and brightest massive star forming molecular clouds, the core of the Orion ne...
A number of stellar streams, moving and kinematic groups were identified in the Milky Way galaxy. So...
Abstract. High-resolution, high signal-to-noise spectral data are presented for four young B-type st...
Due to its proximity, the Orion star forming region is often used as a proxy to study processes rela...
International audienceWe investigate the chemical segregation of complex O-bearing species (includin...
12 pags., 3 apps.We investigate the chemical segregation of complex O-bearing species (including the...
Context. Modern spectroscopy of early-type stars often aims at studying complex physical phenomena ...
Due to its proximity, the Orion star forming region is often used as a proxy to study processes rela...
Abstract. This review discusses recent results on the astrochemistry of (mostly high-mass) star-form...
International audienceWe present a summary of main results from the studies performed in the series ...
Context. Early B-type stars are invaluable indicators of elemental abundances of their bir...
Context. Recent accurate abundance analyses of B-type main sequence stars in the solar vicinity has...
International audience Aims: We re-examine the recombination/collisional emission line (RL/CEL) nebu...
We present non-LTE oxygen abundances for a sample of B stars in the Orion association. The abundance...
Context. The evolution of chemical elements in a galaxy is linked to its star formation history. Var...
As one of the nearest and brightest massive star forming molecular clouds, the core of the Orion ne...
A number of stellar streams, moving and kinematic groups were identified in the Milky Way galaxy. So...
Abstract. High-resolution, high signal-to-noise spectral data are presented for four young B-type st...
Due to its proximity, the Orion star forming region is often used as a proxy to study processes rela...
International audienceWe investigate the chemical segregation of complex O-bearing species (includin...
12 pags., 3 apps.We investigate the chemical segregation of complex O-bearing species (including the...
Context. Modern spectroscopy of early-type stars often aims at studying complex physical phenomena ...
Due to its proximity, the Orion star forming region is often used as a proxy to study processes rela...
Abstract. This review discusses recent results on the astrochemistry of (mostly high-mass) star-form...