Reference : Detection of the inner-debris disk of Vega with CHARA/FLUOR
Scientific congresses and symposiums : Paper published in a book
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
Detection of the inner-debris disk of Vega with CHARA/FLUOR
Absil, Olivier mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS) >]
Di Folco, Emmanuel [Observatoire de Genève (Switzerland)]
Mérand, Antoine [LESIA, Observatoire de Paris - Meudon (France) and CHARA, Georgia State Univ. (USA)]
Augereau, Jean-Charles [Lab. d'Astrophysique de l'Observatoire de Grenoble (France)]
Coudé du Foresto, Vincent [LESIA, Observatoire de Paris - Meudon (France)]
Aufdenberg, Jason P [National Optical Astronomical Observatory (USA)]
Kervella, Pierre [LESIA, Observatoire de Paris - Meudon (France)]
Ridgway, Stephen T [National Optical Astronomical Observatory (USA)]
ten Brummelaar, Theo A [CHARA, Georgia State Univ. (USA)]
McAlister, Harold A [CHARA, Georgia State Univ. (USA)]
Advances in Stellar Interferometry
Monnier, John
Schöller, Markus
Danchi, Willian
Proceedings of the SPIE, volume 6268
Advances in Stellar Interferometry
du 24 au 31 mai 2006
[en] Stars: individual: Vega ; Circumstellar matter ; Techniques: interferometric
[en] Using the FLUOR beam-combiner installed at the CHARA Array (Mt. Wilson, CA), we have obtained highprecision visibility measurements of Vega, one of the prototypic debris-disk stars, known to be surrounded by a large amount of cold dust in a ring-like structure at 80-100 AU. The combination of short and long baselines has allowed us to separately resolve the stellar photosphere and the close environment of the star (less than 8 AU). Our observations show a significant deficit in square visibility at short baselines with respect to the expected visibility of a simple UD stellar model (DeltaV2 equal or equivalent to 2%), suggesting the presence of an extended source of emission around Vega. The sparse (u, v) plane coverage does not allow the discrimination between a point source and an extended circumstellar emission as the source of the extended emission. However, we show that the presence of a point-like source within the FLUOR field-of-view (1" in radius, i.e., 7.8 AU at the distance of Vega) is highly unlikely. The excess emission is most likely due to the presence of hot circumstellar dust in the inner part of Vega's debris disk, with a flux ratio of 1.29 plus or minus 0.19% between the integrated dust emission and the stellar photosphere. Complementing this result with archival photometric data in the near- and mid-infrared and taking into account a realistic photospheric model for the rapidly rotating Vega, we derive the expected physical properties of the circumstellar dust by modelling its Spectral Energy Distribution. The inferred properties suggest that the Vega system could be currently undergoing major dynamical perturbations.
Copyright 2006 Society of Photo-Optical Instrumentation Engineers. One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited.

File(s) associated to this reference

Fulltext file(s):

Open access
vega.pdfAuthor preprint1.13 MBView/Open

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.