Cosmogenic evidence for limited local LGM glacial expansion, Denton Hills, Antarctica

dc.date.accessioned2020-03-11T20:27:04Z
dc.date.accessioned2022-10-18T22:42:15Z
dc.date.available2020-03-11T20:27:04Z
dc.date.available2022-10-18T22:42:15Z
dc.date.created2020-03-11T20:27:04Z
dc.date.issued2017
dc.identifierhttp://hdl.handle.net/10533/238196
dc.identifier15090013
dc.identifierWOS:000418974100007
dc.identifierno scielo
dc.identifiereid=2-s2.0-85033567976
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4469535
dc.description.abstractThe geomorphology of the Denton Hills provides insight into the timing and magnitude of glacial retreats in a region of Antarctica isolated from the influence of the East Antarctic ice sheet. We present 26 Beryllium-10 surface exposure ages from a variety
dc.languageeng
dc.relationhttps://doi.org/10.1016/j.quascirev.2017.11.002
dc.relation10.1016/j.quascirev.2017.11.002
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.titleCosmogenic evidence for limited local LGM glacial expansion, Denton Hills, Antarctica
dc.typeArticulo


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