dc.date.accessioned2020-08-04T21:50:59Z
dc.date.accessioned2022-10-18T23:15:20Z
dc.date.available2020-08-04T21:50:59Z
dc.date.available2022-10-18T23:15:20Z
dc.date.created2020-08-04T21:50:59Z
dc.date.issued2005
dc.identifierhttp://hdl.handle.net/10533/242561
dc.identifier15010003
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4473851
dc.description.abstractIn the framework of the Southern Proper Motion Program, more than 1000 stars have been selected on a proper motion basis to study the structure of the Galactic Thick disk toward the South Galactic Pole. A follow-up program is ongoing to obtain for a large
dc.languageeng
dc.publisherWashington D.C.
dc.relationhttps://www.researchgate.net/publication/252690585_A_study_of_the_Thick_disk_of_the_Galaxy_in_the_direction_of_the_South_Galactic_Pole_in_the_framework_of_the_Southern_Proper_Motion_Program
dc.relationinstname: ANID
dc.relationreponame: Repositorio Digital RI2.0
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.titleA study of the thick disk of the Galaxy in the direction of the South Galactric Pole in the framework of the Southern Proper Motion Program
dc.typeCapitulo de libro


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