Chemical abundances in Orion protoplanetary discs: integral field spectroscopy and photoevaporation models of HST 10

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dc.contributor.authorTsamis, Y.
dc.contributor.authorMesa Delgado, Adal
dc.date.accessioned2016-05-10T18:14:48Z
dc.date.available2016-05-10T18:14:48Z
dc.date.issued2013
dc.identifier.doi10.1093/mnras/stt145
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stt145
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/13440
dc.language.isoen
dc.relation.isformatofMonthly Notices of the Royal Astronomical Society No. 4 (430), p. 3406-3421.
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherDiscos protoplanetarioses_ES
dc.subject.otherNebulosas - Observacioneses_ES
dc.subject.otherFormación Estelares_ES
dc.subject.otherProtoestrellases_ES
dc.titleChemical abundances in Orion protoplanetary discs: integral field spectroscopy and photoevaporation models of HST 10es_ES
dc.typeartículo
sipa.codpersvinculados1010417
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