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dc.contributor.authorRICHARDS, A.M.S.
dc.contributor.authorSOBOLEV, A.
hal.structure.identifierFORMATION STELLAIRE 2019
dc.contributor.authorBAUDRY, Alain
hal.structure.identifierFORMATION STELLAIRE 2019
dc.contributor.authorHERPIN, Fabrice
hal.structure.identifierInstituut voor Sterrenkunde [Leuven]
dc.contributor.authorDECIN, L.
dc.contributor.authorGRAY, M.D.
dc.contributor.authorETOKA, S.
dc.contributor.authorHUMPHREYS, L.
dc.contributor.authorVLEMMINGS, W.
dc.date.issued2019-06
dc.identifier.issn0273-1177
dc.description.abstractEnMaser emission from water, methanol, silicon monoxide and other molecules can reach brightness temperatures K. Such observations can achieve sub-pc precision for discs around black holes or sub-au scale interactions in protostellar discs and the regions where evolved star winds reach escape velocity. Ultra-high resolution maser observations also provide photon statistics, for fundamental physics experiments. RadioAstron has shown the success – and limitations – of cm-wave maser observations on scales mas with sparse baseline coverage. ALMA, APEX and earlier single dish searches have found a wealth of mm and sub-mm masers, some of which probably also attain high brightness temperatures. Masers are ideal for high-resolution observations throughout the radio regime and we need to consider the current lessons for the best observational strategies to meet specific science cases.
dc.language.isoen
dc.publisherElsevier
dc.title.enMasers: Precision probes of molecular gas
dc.typeArticle de revue
dc.identifier.doi10.1016/j.asr.2019.05.052
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique galactique [astro-ph.GA]
bordeaux.journalAdvances in Space Research
bordeaux.pageAdvances in Space Research, Available online 11 June 2019
bordeaux.peerReviewedoui
hal.identifierhal-02164347
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02164347v1
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