Translator Disclaimer
22 June 2006 First astrophysical results from AMBER/VLTI
Author Affiliations +
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.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
F. Malbet, R. G. Petrov, G. Weigelt, P. Stee, E. Tatulli, A. Domiciano de Souza, and F. Millour "First astrophysical results from AMBER/VLTI", Proc. SPIE 6268, Advances in Stellar Interferometry, 626802 (22 June 2006);


CHARA angular diameter measurements with a 330 meter baseline
Proceedings of SPIE (February 21 2003)
The 2008 2009 outburst of the young binary system Z...
Proceedings of SPIE (August 02 2010)
Science program of the AMBER consortium
Proceedings of SPIE (October 20 2004)
Wolf-Rayet stars probed by AMBER/VLTI
Proceedings of SPIE (July 28 2008)

Back to Top