The Globular Cluster M15. I. Identification, Discovery, and Period Determination of Variable Stars

dc.date.accessioned2020-03-11T20:37:56Z
dc.date.accessioned2022-10-18T23:07:11Z
dc.date.available2020-03-11T20:37:56Z
dc.date.available2022-10-18T23:07:11Z
dc.date.created2020-03-11T20:37:56Z
dc.date.issued2008
dc.identifierhttp://hdl.handle.net/10533/241452
dc.identifier15010003
dc.identifierWOS:000254655300030
dc.identifierno scielo
dc.identifiereid=2-s2.0-50849128850
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472791
dc.description.abstractWe present new BVI CCD photometry for variables in the globular cluster M15. Our photometry was obtained using both the image subtraction package ISIS and DAOPHOT/ALLFRAME. The data were acquired in 2001 on two observing runs on 11 observing nights using
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-6256/135/4/1459
dc.relation10.1088/0004-6256/135/4/1459
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe Globular Cluster M15. I. Identification, Discovery, and Period Determination of Variable Stars
dc.typeArticulo


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