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Proceedings Paper

First astrophysical results from AMBER/VLTI
Author(s): F. Malbet; R. G. Petrov; G. Weigelt; P. Stee; E. Tatulli; A. Domiciano de Souza; F. Millour
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Paper Abstract

The AMBER instrument installed at the Very Large Telescope (VLT) combines three beams from as many telescopes to produce spectrally dispersed fringes from milli-arcsecond angular scale in the near infrared. Two years after installation, first scientific observations have been carried out during the Science Demonstration Time and the Guaranteed Time mostly on bright sources due to some VLTI limitations. In this paper, we review these first astrophysical results and we show which types of completely new information is brought by AMBER. The first astrophysical results have been mainly focusing on stellar wind structure, kinematics, and its interaction with dust usually concentrated in a disk. Because AMBER has dramatically increased the number of measures per baseline, this instrument brings strong constraints on morphology and models despite a relatively poor (u,v) coverage for each object.

Paper Details

Date Published: 22 June 2006
PDF: 8 pages
Proc. SPIE 6268, Advances in Stellar Interferometry, 626802 (22 June 2006); doi: 10.1117/12.673100
Show Author Affiliations
F. Malbet, Lab. d'Astrophysique de Grenoble (France)
R. G. Petrov, Lab. Univ. d'Astrophysique de Nice (France)
G. Weigelt, Max-Planck Institut für Astrophysick (Germany)
P. Stee, Observatoire de la Côte d'Azur (France)
E. Tatulli, Osservatorio Astrofisico di Arcetri (Italy)
A. Domiciano de Souza, Lab. Univ. d'Astrophysique de Nice (France)
Observatoire de la Côte d'Azur (France)
F. Millour, Lab. d'Astrophysique de Grenoble (France)
Lab. Univ. d'Astrophysique de Nice (France)


Published in SPIE Proceedings Vol. 6268:
Advances in Stellar Interferometry
John D. Monnier; Markus Schöller; William C. Danchi, Editor(s)

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