On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0─2.5

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dc.contributor.authorZavala, Jorge A.
dc.contributor.authorCasey, Caitlin M.
dc.contributor.authorScoville, Nick Z.
dc.contributor.authorChampagne, Jaclyn B.
dc.contributor.authorChiang, Y.
dc.contributor.authorDannerbauer, H.
dc.contributor.authorDrew, P.
dc.contributor.authorFu, Hai
dc.contributor.authorSpilker, J.
dc.contributor.authorTreister, Ezequiel
dc.date.accessioned2020-08-13T23:19:30Z
dc.date.available2020-08-13T23:19:30Z
dc.date.issued2019
dc.date.updated2020-08-13T17:40:44Z
dc.fuente.origenORCID
dc.identifier.doi10.3847/1538-4357/ab5302
dc.identifier.issn0004-637X
dc.identifier.urihttps://doi.org/10.3847/1538-4357/ab5302
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/38903
dc.issue.numeroNo. 2
dc.language.isoen
dc.pagina.final15
dc.pagina.inicio1
dc.relation.isformatofThe Astrophysical journal, vol. 887, no. 2 (dic., 2019), pp.1-15
dc.revistaThe Astrophysical journales_ES
dc.subjectAstronomíaes_ES
dc.subjectGalaxias apagadases_ES
dc.subjectAstronomía submilimétricaes_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.titleOn the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0─2.5es_ES
dc.typeartículo
dc.volumenVol. 887
sipa.codpersvinculados1031846
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