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Infrared Interferometric Gravity Darkening Observations of Vega with CHARA/FLUOR
Aufdenberg, J.; Mérand, A.; Coudé Du Foresto, V. et al.
2006In Coudé du Foresto, Vincent; Rouan, Daniel; Rousset, Gérard (Eds.) Visions for Infrared Astronomy
 

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Keywords :
Vega; interferometry; stellar atmospheres; stellar rotation; fundamental stellar parameters.
Abstract :
[en] We have obtained high-precision measurements of Vega at projected baselines between 103 m and 273 m with the CHARA Array using the (FLUOR) beam combiner in the K' band. A strongly gravity-darkened model atmosphere is in general agreement with both our interferometric data and archival spectrophotometry. This model indicates that Vega is rotating at 91%ofitsangular break-uprateandthatthepole-to-equator effectivetemperaturedifference is 2250 K.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Aufdenberg, J.
Mérand, A.
Coudé Du Foresto, V.
Absil, Olivier  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
di Folco, E.
Kervella, P.
Ridgway, S.
Berger, D.
Ten Brummelaar, T.
McAlister, H.
Sturmann, J.
Turner, N.
Language :
English
Title :
Infrared Interferometric Gravity Darkening Observations of Vega with CHARA/FLUOR
Publication date :
March 2006
Event name :
Visions for Infrared Astronomy
Event organizer :
Rouan D. & Ridgway S.
Event place :
Paris, France
Event date :
du 20 au 22 mars 2006
Audience :
International
Main work title :
Visions for Infrared Astronomy
Editor :
Coudé du Foresto, Vincent
Rouan, Daniel
Rousset, Gérard
Publisher :
Lavoisier, Paris, France
Collection name :
Instrumentation, Mesure, Métrologie vol 6/1-4
Pages :
305-308
Available on ORBi :
since 25 January 2012

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