Add to ORKGSulfur is an abundant element which remains undepleted in diffuse interstellar gas (Av<1) but it is traditionally assumed to deplete on dust grains at higher densities and larger Av. Photodissociation regions (PDRs) are an interesting intermediate medium between translucent and dark clouds where the chemistry and energetics are dominated by the illuminating FUV radiation field. Thus they can provide new insights about the sulfur depletion problem. However, physical and chemical gradients in PDRs take place at small angular scales (~1 to 10''). Aperture synthesis observations are therefore required to resolve such gradients. Besides, a complete understanding of molecular excitation is needed to correctly determine molecular abundances but al...
Context. The sulfur abundance is poorly known in most environments. Yet, deriving the sulfur abundan...
Accepted by Astronomy & Astrophysics 2018 (15 pages, 15 figures, 8 tables)International audienceCont...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...
Aims.We present $3.65''$ $\times$ $3.34''$ angular-resolution IRAM Plateau de Bure Interferometer (...
International audienceHydride molecules lie at the base of interstellar chemistry, but the synthesis...
Context. Sulphur is one of the most abundant elements in the Universe (S/H ~ 1.3 × 10−5) and plays a...
The main carrier of sulfur in dense clouds, where it is depleted from the gas phase, remains a myste...
International audienceAims. Our goal is to complete the inventory of S-bearing molecules and their a...
Context. A fraction of the missing sulfur in dense clouds and circumstellar regions could be in the ...
A longstanding problem in astrochemistry is the inability of many current models to account for miss...
In this work, we reexamine sulfur chemistry occurring on and in the ice mantles of interstellar dust...
Sulfur has been observed to be severely depleted in dense clouds leading to uncertainty in the molec...
International audienceWe present the first detection of gas phase S2H in the Horsehead, a moderately...
Context. The sulfur abundance is poorly known in most environments. Yet, deriving the sulfur abundan...
Accepted by Astronomy & Astrophysics 2018 (15 pages, 15 figures, 8 tables)International audienceCont...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...
Aims.We present $3.65''$ $\times$ $3.34''$ angular-resolution IRAM Plateau de Bure Interferometer (...
International audienceHydride molecules lie at the base of interstellar chemistry, but the synthesis...
Context. Sulphur is one of the most abundant elements in the Universe (S/H ~ 1.3 × 10−5) and plays a...
The main carrier of sulfur in dense clouds, where it is depleted from the gas phase, remains a myste...
International audienceAims. Our goal is to complete the inventory of S-bearing molecules and their a...
Context. A fraction of the missing sulfur in dense clouds and circumstellar regions could be in the ...
A longstanding problem in astrochemistry is the inability of many current models to account for miss...
In this work, we reexamine sulfur chemistry occurring on and in the ice mantles of interstellar dust...
Sulfur has been observed to be severely depleted in dense clouds leading to uncertainty in the molec...
International audienceWe present the first detection of gas phase S2H in the Horsehead, a moderately...
Context. The sulfur abundance is poorly known in most environments. Yet, deriving the sulfur abundan...
Accepted by Astronomy & Astrophysics 2018 (15 pages, 15 figures, 8 tables)International audienceCont...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...