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dc.date.accessioned 2010-10-04T21:26:43Z
dc.date.available 2010-10-04T03:00:00Z
dc.date.issued 1998
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/2088
dc.description.abstract The aim of the present paper is to discuss the significance, in the infrared continuum of Be stars, of the dielectronic recombination (DR) of Mg II atoms. To accomplish this, we hace calculated the emissitivity in the lines of Mg I atoms after the process of electron capture has taken place. In order to estimate its influence in the photospheric flux, we have considered the total energy emitted in all lines with λ1 ≤ λ ≤ λ2, where λ1 and λ2 define the wavelegth ranges of the Johnson system filters. We conclude that the DR of Mg II atoms does actually contribute significantly to the infrared excess observed in Be stars. en
dc.format.extent 902-915 es
dc.language en es
dc.subject estrellas es
dc.subject atomic processes; emission line; Be stars es
dc.subject astrofísica es
dc.title Dielectronic recombination of Mg II in stellar envelopes en
dc.type Articulo es
sedici.identifier.uri http://iopscience.iop.org/article/10.1086/306004 es
sedici.identifier.issn 0004-637X es
sedici.creator.person Cruzado, Alicia es
sedici.creator.person Di Rocco, Héctor Oscar es
sedici.creator.person Ringuelet, Adela Emilia 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-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-nd/4.0/
sedici.description.peerReview peer-review es
sedici2003.identifier ARG-UNLP-ART-0000006633 es
sedici.relation.journalTitle The Astrophysical Journal es
sedici.relation.journalVolumeAndIssue vol. 503, no. 2 es

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