Toward precise ages for single stars in the field. Gyrochronology constraints at several Gyr using wide binaries. I. Ages for initial sample

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dc.contributor.authorChanamé, Julio
dc.date.accessioned2016-05-10T18:02:25Z
dc.date.available2016-05-10T18:02:25Z
dc.date.issued2012
dc.identifier.doi10.1088/0004-637X/746/1/102
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/12252
dc.identifier.urihttps://doi.org/10.1088/0004-637X/746/1/102
dc.identifier.wosidWOS:000302861300102
dc.language.isoen
dc.nota.accesocontenido completo
dc.pagina.final15
dc.pagina.inicio1
dc.relation.isformatofAstrophysical Journal Vol. 746, No. 1, Art. 102.
dc.revistaAstrophysical Journales_ES
dc.rightsacceso abierto
dc.subject.ddc520
dc.subject.deweyAstronomíaes_ES
dc.subject.otherEstrellas - Rtotaciónes_ES
dc.subject.otherEstrellas Evoluciónes_ES
dc.subject.otherAstronomía - Observacioneses_ES
dc.titleToward precise ages for single stars in the field. Gyrochronology constraints at several Gyr using wide binaries. I. Ages for initial samplees_ES
dc.typeartículo
dc.volumenVol. 746
sipa.codpersvinculados104380
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