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Complex organic molecules toward low-mass and high-mass star forming regions

hal.structure.identifierEquipe de Recherche en Ingénierie des Connaissances [ERIC]
dc.contributor.authorFAVRE, C.
hal.structure.identifierKarlsruhe Institute of Technology [KIT]
dc.contributor.authorCECCARELLI, C.
dc.contributor.authorLEFLOCH, B.
hal.structure.identifierDepartment of Astronomy [Ann Arbor]
dc.contributor.authorBERGIN, E.
dc.contributor.authorCARVAJAL, M.
hal.structure.identifierFORMATION STELLAIRE 2016
dc.contributor.authorBROUILLET, N.
hal.structure.identifierFORMATION STELLAIRE 2016
dc.contributor.authorDESPOIS, D.
hal.structure.identifierforeign laboratories [FL]
dc.contributor.authorJØRGENSEN, J.
hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorKLEINER, I.
dc.date.issued2016-12
dc.date.conference2016-06-14
dc.description.abstractEnOne of the most important questions in molecular astrophysics is how, when, and where complex organic molecules, COMs (≥ 6 atoms) are formed. In the Interstellar-Earth connection context, could this have a bearing on the origin of life on Earth? Formation mechanisms of COMs, which include potentially prebiotic molecules, are still debated and may include grain-mantle and/or gas-phase chemistry. Understanding the mechanisms that lead to the interstellar molecular complexification, along with the involved physicochemical processes, is mandatory to answer the above questions. In that context, active researches are ongoing in theory, laboratory experiment, chemical modeling and observations. Thanks to recent progress in radioastronomy instrumentation for both single-dish and millimeter array (e.g. Herschel, NOEMA, ALMA), new results have been obtained. I will review some notable results on the detection of COMs, including prebiotic molecules, towards star forming regions.
dc.language.isoen
dc.subject.enastrochemistry
dc.subject.enISM: molecules
dc.subject.enSubmillimeter: ISM
dc.title.enComplex organic molecules toward low-mass and high-mass star forming regions
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.page321 - 325
bordeaux.countryFR
bordeaux.conference.cityLyon
bordeaux.peerReviewedoui
hal.identifierhal-01462860
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2016-06-17
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01462860v1
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