Is a binary fraction-age relation responsible for the lack of EHB binaries in globular clusters?

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dc.contributor.authorMoni Bidin, C.
dc.contributor.authorCatelan, Márcio
dc.date.accessioned2017-04-11T20:51:43Z
dc.date.available2017-04-11T20:51:43Z
dc.date.issued2008
dc.identifier.issn0004-6361
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/19149
dc.language.isoen
dc.relation.isformatofAstronomy & Astrophysics. Vol. 480, no. 1 (2008), p. [L1]-L4
dc.revistaAstronomy & Astrophysicses_ES
dc.rightsacceso restringido
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas enanases_ES
dc.subject.otherEspectroscopía astronómicaes_ES
dc.titleIs a binary fraction-age relation responsible for the lack of EHB binaries in globular clusters?es_ES
dc.typeartículo
sipa.codpersvinculados1001556
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