The mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Survey

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dc.contributor.authorZhou, G.
dc.contributor.authorBayliss, D.
dc.contributor.authorHartman, J.
dc.contributor.authorBakos, G.
dc.contributor.authorPenev, K.
dc.contributor.authorCsubry, Z.
dc.contributor.authorTan, T.
dc.contributor.authorJordán Colzani, Andrés Cristóbal
dc.contributor.authorMancini, L.
dc.contributor.authorRabus, Markus
dc.date.accessioned2020-10-09T01:24:06Z
dc.date.available2020-10-09T01:24:06Z
dc.date.issued2014
dc.format.extent14 páginas
dc.fuente.origenConveris
dc.identifier.doi10.1093/mnras/stt2100
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.urihttps://doi.org/10.1093/mnras/stt2100
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/47146
dc.identifier.wosidWOS:000329158900062
dc.issue.numeroNo. 3
dc.language.isoen
dc.pagina.final2844
dc.pagina.inicio2831
dc.revistaMonthly Notices of the Royal Astronomical Societyes_ES
dc.rightsacceso restringido
dc.subject.ods13 Climate action
dc.subject.odspa13 Acción por el clima
dc.titleThe mass-radius relationship for very low mass stars: Four new discoveries from the HATSouth Surveyes_ES
dc.typeartículo
dc.volumenVol. 437
sipa.codpersvinculados176960
sipa.codpersvinculados1008065
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