Context. Hydrogen recombination emission lines commonly observed in accreting young stellar objects represent a powerful tracer for the gas conditions in the circumstellar structures (accretion columns, and winds or jets). Aims. Here we perform a study of the H
International audienceContext: Hydrides of the most abundant heavier elements are fundamental molecu...
International audienceRecent achievements of laboratory astrophysics experiments with high power las...
Contains fulltext : 84454.pdf (preprint version ) (Open Access
The hydrogen emission line is a defining characteristic of young stellar objects probing the planet ...
SIGLEAvailable from British Library Document Supply Centre-DSC:DXN030108 / BLDSC - British Library D...
We have analysed the infrared hydrogen recombination lines of a sample of well studied hot massive s...
We present VLT/X-shooter observations of a sample of 36 accreting low-mass stellar and substellar ob...
Context: Young stars grow by accreting gas from a circumstellar disk. These stars also possess stron...
Aims.Optical and near-infrared spectroscopy of molecular hydrogen in interstellar shocks provide a v...
We present new medium-resolution longslit spectra in the near-infrared and examine the excitation of...
We are trying to probe conditions in the youngest super star clusters, those still embedded in dens...
International audienceWe present new results of a spectroscopic survey of circumstellar H I in the d...
Type article Title Hydrogen infrared recombination lines as a diagnostic tool for the geometry of th...
International audienceContext: Hydrides of the most abundant heavier elements are fundamental molecu...
International audienceRecent achievements of laboratory astrophysics experiments with high power las...
Contains fulltext : 84454.pdf (preprint version ) (Open Access
The hydrogen emission line is a defining characteristic of young stellar objects probing the planet ...
SIGLEAvailable from British Library Document Supply Centre-DSC:DXN030108 / BLDSC - British Library D...
We have analysed the infrared hydrogen recombination lines of a sample of well studied hot massive s...
We present VLT/X-shooter observations of a sample of 36 accreting low-mass stellar and substellar ob...
Context: Young stars grow by accreting gas from a circumstellar disk. These stars also possess stron...
Aims.Optical and near-infrared spectroscopy of molecular hydrogen in interstellar shocks provide a v...
We present new medium-resolution longslit spectra in the near-infrared and examine the excitation of...
We are trying to probe conditions in the youngest super star clusters, those still embedded in dens...
International audienceWe present new results of a spectroscopic survey of circumstellar H I in the d...
Type article Title Hydrogen infrared recombination lines as a diagnostic tool for the geometry of th...
International audienceContext: Hydrides of the most abundant heavier elements are fundamental molecu...
International audienceRecent achievements of laboratory astrophysics experiments with high power las...
Contains fulltext : 84454.pdf (preprint version ) (Open Access
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