Resetting chemical clocks of hot cores based on S-bearing molecules
A&A, 422 1 (2004) 159-169
Published online: 2004-07-06
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A study of the region of massive star formation L379IRS1 in radio lines of methanol and other molecules
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Laboratory microwave, millimeter wave and far-infrared spectra of dimethyl sulfide
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CHEMICAL DIAGNOSTICS OF THE MASSIVE STAR CLUSTER-FORMING CLOUD G33.92+0.11. I. 13CS, CH3OH, CH3N, OCS, H2S, SO2, and SiO
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Detection of CH3SH in protostar IRAS 16293-2422
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Sulfur-bearing molecules observed in the massive star-forming regions, DR21(OH) and G33.92+0.11
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A new study of an old sink of sulphur in hot molecular cores: the sulphur residue
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Resolving the chemical substructure of Orion-KL
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The density structure of the L1157 molecular outflow★†
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SUBMILLIMETER ARRAY HIGH-ANGULAR RESOLUTION OBSERVATIONS OF THE MONOCEROS R2 STAR-FORMING CLUSTER
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Sulphur depletion in dense clouds and circumstellar regions. Organic products made from UV photoprocessing of realistic ice analogs containing H2S
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Modelling the chemical evolution of molecular clouds as a function of metallicity
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EXCLUSION OF COSMIC RAYS IN PROTOPLANETARY DISKS. II. CHEMICAL GRADIENTS AND OBSERVATIONAL SIGNATURES
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Theoretical spectroscopic characterization at low temperatures of detectable sulfur-organic compounds: Ethyl mercaptan and dimethyl sulfide
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A high-resolution study of complex organic molecules in hot cores
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Theoretical spectroscopic characterization at low temperatures of S-methyl thioformate and O-methyl thioformate
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