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Spectroscopic and interferometric approach for differential rotation in massive fast rotators

Document type: Comunicacion

Abstract

The 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.

General information

Issue date: julio 2011
Document language: English
Journal: Proceedings of the International Astronomical Union; vol. 6, no. S272
Event: IAU Symposium 272 (Paris, France, 19-23 July, 2010)
Origin: Facultad de Ciencias Astronómicas y Geofísicas
ISSN: 1743-9213
Pages: 103-105
xmlui.dri2xhtml.METS-1.0.item-dc-subject: Stars: rotation ; Techniques: interferometric ; Techniques: spectroscopic
Subjects: Ciencias Astronómicas

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Created: 25 de octubre de 2019
Available since: 25 de octubre de 2019
Please, use one of this identificators(URI) for cite o linking this item:
  • http://sedici.unlp.edu.ar/handle/10915/84073
  • https://doi.org/10.1017/s1743921311010118

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    Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)