Relation between halo spin and cosmic-web filaments at z similar or equal to 3

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dc.contributor.authorGonzález Reyes, Roberto
dc.contributor.authorPrieto, Joaquin
dc.contributor.authorPadilla, Nelson
dc.contributor.authorJimenez, Raul
dc.date.accessioned2020-06-30T21:22:20Z
dc.date.available2020-06-30T21:22:20Z
dc.date.issued2017
dc.format.extent7 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stw2715
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/stw2715
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/30147
dc.issue.numeroNo. 4
dc.language.isoen
dc.pagina.final4672
dc.pagina.inicio4666
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherGalaxiases_ES
dc.subject.otherMateria oscura (astronomía)es_ES
dc.subject.otherAstrofísicaes_ES
dc.titleRelation between halo spin and cosmic-web filaments at z similar or equal to 3es_ES
dc.typeartículo
dc.volumenVol. 464
sipa.codpersvinculados17891
sipa.codpersvinculados1003598
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