International audienceWe present the first detection of gas phase S2H in the Horsehead, a moderately UV-irradiated nebula. This confirms the presence of doubly sulfuretted species in the interstellar medium and opens a new challenge for sulfur chemistry. The observed S2H abundance is ~5x10$^{-11}$, only a factor 4-6 lower than that of the widespread H2S molecule. H2S and S2H are efficiently formed on the UV-irradiated icy grain mantles. We performed ice irradiation experiments to determine the H2S and S2H photodesorption yields. The obtained values are ~1.2x10$^{-3}$ and <1x10$^{-5}$ molecules per incident photon for H2S and S2H, respectively. Our upper limit to the S2H photodesorption yield suggests that photo-desorption is not a competiti...
International audienceSulphur-bearing molecules are highly reactive in the gas phase of the interste...
Context. A fraction of the missing sulfur in dense clouds and circumstellar regions could be in the ...
International audienceAims. Our goal is to complete the inventory of S-bearing molecules and their a...
International audienceWe present the first detection of gas phase S2H in the Horsehead, a moderately...
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. Surprisingly, sulphuretted mo...
Context. Sulphur is one of the most abundant elements in the Universe (S/H ~ 1.3 × 10−5) and plays a...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...
International audienceSulfur is of fundamental importance in a wide variety of phenomena such as lif...
International audienceSulphur-bearing molecules are highly reactive in the gas phase of the interste...
Context. A fraction of the missing sulfur in dense clouds and circumstellar regions could be in the ...
International audienceAims. Our goal is to complete the inventory of S-bearing molecules and their a...
International audienceWe present the first detection of gas phase S2H in the Horsehead, a moderately...
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. Surprisingly, sulphuretted mo...
Context. Sulphur is one of the most abundant elements in the Universe (S/H ~ 1.3 × 10−5) and plays a...
Aims. This work aims to study the unexplained sulfur depletion observed toward dense clouds and prot...
International audienceSulfur is of fundamental importance in a wide variety of phenomena such as lif...
International audienceSulphur-bearing molecules are highly reactive in the gas phase of the interste...
Context. A fraction of the missing sulfur in dense clouds and circumstellar regions could be in the ...
International audienceAims. Our goal is to complete the inventory of S-bearing molecules and their a...