The evolution of the baryon fraction in haloes as a cause of scatter in the galaxy stellar mass in the EAGLE simulation

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dc.contributor.authorKulier, Andrea
dc.contributor.authorPadilla, Nelson
dc.contributor.authorSchaye, J.
dc.contributor.authorCrain, R. A.
dc.contributor.authorSchaller, M.
dc.contributor.authorBower, R. G.
dc.contributor.authorTheuns, T.
dc.contributor.authorPaillas Villavicencio, Enrique
dc.date.accessioned2021-05-31T03:45:19Z
dc.date.available2021-05-31T03:45:19Z
dc.date.issued2019
dc.format.extent13 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/sty2914
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/sty2914
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/60149
dc.language.isoen
dc.nota.accesoContenido parcial
dc.pagina.final3273
dc.pagina.inicio3261
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso restringido
dc.titleThe evolution of the baryon fraction in haloes as a cause of scatter in the galaxy stellar mass in the EAGLE simulationes_ES
dc.typeartículo
dc.volumenVol. 482
sipa.codpersvinculados1058413
sipa.codpersvinculados1003598
sipa.codpersvinculados249896
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