6533b82afe1ef96bd128cc04
RESEARCH PRODUCT
Laboratory measurements and astronomical search for the HSO radical
Cristina PuzzariniTill KirschJosé CernicharoBelén TerceroGabriele CazzoliJürgen GaussValerio Lattanzisubject
inorganic chemicalsMethods: laboratory: molecularHydrogenLine: identificationlaboratory: molecular [Methods]chemistry.chemical_elementContext (language use)ISM: moleculeAstrophysics7. Clean energy01 natural sciencesArticleAbundance (ecology)0103 physical sciencesPhysics::Chemical Physicsidentification [Line]Spectral resolutionSubmillimeter: ISM010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmolecules [ISM]Radio lines: ISMPhysics010304 chemical physicsMolecular dataTriatomic moleculeISM [Submillimeter]AstronomyAstronomy and AstrophysicsAstronomy and AstrophysicSulfurDiatomic moleculeISM: moleculesISM [Radio lines]Interstellar mediumchemistry13. Climate actionSpace and Planetary Sciencedescription
[Context] Despite the fact that many sulfur-bearing molecules, ranging from simple diatomic species up to astronomical complex molecules, have been detected in the interstellar medium, the sulfur chemistry in space is largely unknown and a depletion in the abundance of S-containing species has been observed in the cold, dense interstellar medium. The chemical form of the missing sulfur has yet to be identified.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2016-01-01 | Astronomy & Astrophysics |