Spectroscopic and interferometric approach for differential rotation in massive fast rotators

dc.creatorZorec, Juan
dc.creatorFrémat, Yves
dc.creatorDelaa, Omar
dc.creatorDe Souza, Armando Domiciano
dc.creatorStee, Philippe
dc.creatorMourard, Denis
dc.creatorCidale, Lydia Sonia
dc.creatorMartayan, Christophe
dc.date2011-07
dc.date2019-10-25T15:15:11Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/84073
dc.identifierissn:1743-9213
dc.descriptionThe coupling between the convective region in the envelope and rotation can produce a surface latitudinal differential rotation that may induce changes of the stellar geometry and on the spectral line profiles that it may be scrutinized spectroscopically and by interferometry.
dc.descriptionFacultad de Ciencias Astronómicas y Geofísicas
dc.formatapplication/pdf
dc.format103-105
dc.languageen
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectStars: rotation
dc.subjectTechniques: interferometric
dc.subjectTechniques: spectroscopic
dc.titleSpectroscopic and interferometric approach for differential rotation in massive fast rotators
dc.typeArticulo
dc.typeComunicacion


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