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dc.contributor.authorMAJUMDAR, Liton
hal.structure.identifierAMOR 2018
dc.contributor.authorWAKELAM, Valentine
hal.structure.identifierAMOR 2018
dc.contributor.authorGRATIER, P.
hal.structure.identifierCentre d'étude spatiale des rayonnements [CESR]
dc.contributor.authorCAUX, Emmanuel
dc.contributor.authorWILLACY, Karen
dc.contributor.authorRESSLER, M. E.
dc.date.issued2018
dc.date.conference2018-07-14
dc.description.abstractEnObservation of CO2 in exoplanet atmospheres is one of the major science themes for James Webb Space Telescope (JWST). CO2 cannot be observed in the gas phase through rotational transitions in the far-infrared or submillimeter range due to its lack of permanent dipole moment. It has to be observed through its vibrational transitions at near- and mid-infrared wavelengths. We will show how observation of protonated form of CO2 in a solar-type protostar help us to better understand the overall temperature structure, ionization structure, H2O and CO2 snow lines, and overall C/O ratio. Implications of our study to the chemistry of CO2 ices using JWST-MIRI and NIRSpec will be discussed as well.
dc.language.isoen
dc.title.enChemistry in Protostellar regions: New implications for JWST MIRI/NIRSpec
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
bordeaux.conference.title42nd COSPAR Scientific Assembly. Held 14-22 July 2018, in Pasadena, California, USA, Abstract id. E1.18-18-18
bordeaux.countryUS
bordeaux.conference.citypasadena
bordeaux.peerReviewedoui
hal.identifierhal-01901848
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2018-07-22
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01901848v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=MAJUMDAR,%20Liton&WAKELAM,%20Valentine&GRATIER,%20P.&CAUX,%20Emmanuel&WILLACY,%20Karen&rft.genre=unknown


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