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dc.contributor.authorMAJUMDAR, M
hal.structure.identifierAMOR 2018
dc.contributor.authorGRATIER, P.
hal.structure.identifierAMOR 2018
dc.contributor.authorWAKELAM, Valentine
dc.contributor.authorCAUX, M
dc.contributor.authorWILLACY, K
dc.contributor.authorRESSLER, M
dc.date.issued2018-03-15
dc.identifier.issn0035-8711
dc.description.abstractEnThe protonated form of CO2, HOCO+, is assumed to be an indirect tracer of CO2 in the millimeter/submillimeter regime since CO2 lacks a permanent dipole moment. Here, we report the detection of two rotational emission lines (40, 4-30, 3 and 50, 5-40, 4) of HOCO+ in IRAS 16293-2422. For our observations, we have used EMIR heterodyne 3 mm receiver of the IRAM 30m telescope. The observed abundance of HOCO+ is compared with the simulations using the 3-phase NAUTILUS chemical model. Implications of the measured abundances of HOCO+ to study the chemistry of CO2 ices using JWST-MIRI and NIRSpec are discussed as well.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.title.enDetection of HOCO+ in the protostar IRAS 16293-2422
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/sty703
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv1803.05442
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page525-530
bordeaux.volume477
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-01742764
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01742764v1
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