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dc.date.accessioned 2019-11-13T18:55:21Z
dc.date.available 2019-11-13T18:55:21Z
dc.date.issued 2013
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/85567
dc.description.abstract NGC 6791 is an open cluster that it is so close to us that can be imaged down to very faint luminosities. The main sequence turn-off age (∼8 Gyr) and the age derived from the cut-off of the white dwarf luminosity function (∼6 Gyr) were found to be significantly different. Here we demonstrate that the origin of this age discrepancy lies in an incorrect evaluation of the white dwarf cooling ages, and we show that when the relevant physical separation processes are included in the calculation of white dwarf sequences both ages are coincident. en
dc.language en es
dc.subject white dwarfs es
dc.title A consistency test of white dwarf and main sequence ages: NGC 6791 en
dc.type Articulo es
sedici.identifier.other doi:10.1051/epjconf/20134305003 es
sedici.identifier.other eid:2-s2.0-84875644547 es
sedici.identifier.issn 2101-6275 es
sedici.creator.person García Berro, E. es
sedici.creator.person Torres, S. es
sedici.creator.person Isern, J. es
sedici.creator.person Salaris, M. es
sedici.creator.person Córsico, Alejandro Hugo es
sedici.creator.person Althaus, Leandro Gabriel es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc/4.0/
sedici.relation.event 40th Liege International Astrophysical Colloquium. Ageing Low Mass Stars: From Red Giants to White Dwarfs (Liège, Belgium, July 9-13, 2012) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle EPJ Web of Conferences es
sedici.relation.journalVolumeAndIssue vol. 43 es


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Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)