Structure and Composition of Two Transitional Circumstellar Disks in Corona Australis

dc.date.accessioned2020-03-11T20:35:56Z
dc.date.accessioned2022-10-18T23:02:14Z
dc.date.available2020-03-11T20:35:56Z
dc.date.available2022-10-18T23:02:14Z
dc.date.created2020-03-11T20:35:56Z
dc.date.issued2010
dc.identifierhttp://hdl.handle.net/10533/240800
dc.identifier15010003
dc.identifierWOS:000280882300019
dc.identifierno scielo
dc.identifiereid=2-s2.0-78049277343
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472139
dc.description.abstractThe late stages of evolution of the primordial circumstellar disks surrounding young stars are poorly understood, yet vital to constrain theories of planet formation. We consider basic structural models for the disks around two ~10 Myr-old members of the
dc.languageeng
dc.relationhttps://doi.org/10.1088/0004-6256/140/3/887
dc.relation10.1088/0004-6256/140/3/887
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.titleStructure and Composition of Two Transitional Circumstellar Disks in Corona Australis
dc.typeArticulo


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