Using Line Profiles to Test the Fraternity of Type Ia Supernovae At High and Low Redshifts

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dc.contributor.authorBlondin, S.
dc.contributor.authorClocchiatti, Alejandro
dc.date.accessioned2017-04-10T20:44:45Z
dc.date.available2017-04-10T20:44:45Z
dc.date.issued2006
dc.identifier.doi10.1086/498724
dc.identifier.issn0004-6256
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/18095
dc.identifier.urihttps://doi.org/10.1086/498724
dc.language.isoen
dc.nota.accesoContenido completo
dc.relation.isformatofAstronomical Journal. Vol. 131, no. 3 (2006), p. [1648]-1666
dc.revistaAstronomical Journales_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherSupernovas (Astronomía)Astronomía - Observacioneses_ES
dc.titleUsing Line Profiles to Test the Fraternity of Type Ia Supernovae At High and Low Redshiftses_ES
dc.typeartículo
dc.volumenVol. 131
sipa.codpersvinculados100500
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