The delay of shock breakout due to circumstellar material evident in most type II supernovae

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dc.contributor.authorForster, F.
dc.contributor.authorMoriya, T. J.
dc.contributor.authorMaureira, J. C.
dc.contributor.authorAnderson, J. P.
dc.contributor.authorBlinnikov, S.
dc.contributor.authorBufano, F.
dc.contributor.authorCabrera Vives, G.
dc.contributor.authorClocchiatti, Alejandro
dc.contributor.authorDe Jaeger, T.
dc.contributor.authorEstevez, P. A.
dc.contributor.authorGalbany, L.
dc.contributor.authorGonzález -Gaitán, S.
dc.contributor.authorGrafener, G.
dc.contributor.authorHamuy, M.
dc.contributor.authorHsiao, E. Y.
dc.contributor.authorHuentelemu, P.
dc.contributor.authorHuijse, P.
dc.contributor.authorKuncarayakti, H.
dc.contributor.authorMartínez, J.
dc.contributor.authorMedina, G.
dc.contributor.authorOlivares, F.
dc.contributor.authorPignata, Giuliano
dc.contributor.authorRazza, A.
dc.contributor.authorReyes, I.
dc.contributor.authorSan Martín, J.
dc.contributor.authorSmith, R. C.
dc.contributor.authorVera, E.
dc.contributor.authorVivas, A. K.
dc.contributor.authorPostigo, A. D.
dc.contributor.authorYoon, S. C.
dc.contributor.authorAshall, C.
dc.contributor.authorFraser, M.
dc.contributor.authorGal-Yam, A.
dc.contributor.authorKankare, E.
dc.contributor.authorLe Guillou, L.
dc.contributor.authorMazzali, P. A.
dc.contributor.authorWalton, N. A.
dc.contributor.authorYoung, D. R.
dc.date.accessioned2021-05-31T03:45:13Z
dc.date.available2021-05-31T03:45:13Z
dc.date.issued2018
dc.format.extent11 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1038/s41550-018-0563-4
dc.identifier.doi10.1038/s41550-018-0563-4
dc.identifier.eissn2397-3366
dc.identifier.issn2397-3366
dc.identifier.urihttps://doi.org/10.1038/s41550-018-0563-4
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/60120
dc.issue.numeroNo. 10
dc.language.isoen
dc.nota.accesoContenido parcial
dc.pagina.final818
dc.pagina.inicio808
dc.revistaNature Astronomyes_ES
dc.rightsacceso restringido
dc.titleThe delay of shock breakout due to circumstellar material evident in most type II supernovaees_ES
dc.typeartículo
dc.volumenVol. 2
sipa.codpersvinculados100500
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