New evidence supporting membership for TW nor in lynga 6 and the centaurus spiral arm

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dc.contributor.authorMajaess, D.
dc.contributor.authorMinniti, D.
dc.contributor.authorKalbusch Saito, Roberto
dc.date.accessioned10-05-2016 15:16
dc.date.available10-05-2016 15:16
dc.date.issued2011
dc.identifier.doi10.1088/2041-8205/741/2/L27
dc.identifier.issn2041-8205
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/14321
dc.identifier.urihttps://doi.org/10.1088/2041-8205/741/2/L27
dc.identifier.wosidWOS:000296753100003
dc.language.isoen
dc.nota.accesoContenido completo
dc.relation.isformatofThe Astrophysical Journal Letters No. 2 (741), Art. L27.
dc.revistaThe Astrophysical Journal Letters
dc.subject.ddc520
dc.subject.deweyAstronomía
dc.subject.otherGalaxias
dc.subject.otherEstrellas - Cúmulos
dc.subject.otherEstrellas variables
dc.subject.otherCefeidas
dc.titleNew evidence supporting membership for TW nor in lynga 6 and the centaurus spiral arm
dc.typeartículo
sipa.codpersvinculados100504
sipa.codpersvinculados1007687
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