Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..315t&link_type=abstract
SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli
Astronomy and Astrophysics
Astrophysics
Scientific paper
The young stellar object MWC 297, which exhibits strong hydrogen emission lines and a strong near infrared continuum excess, has been observed by the AMBER/VLTI instrument on a 47 m baseline in the K spectral band centered around the Brγ line at 2.1656 microns. The object has been resolved in the continuum and in the Brγ line where the flux is about twice larger with a visibility about twice smaller. Thanks to the combination of these AMBER measurements with existing optical and NIR spectra and existing interferometric NIR continuum measurements, a global picture of this intriguing object emerges in which MWC 297 is surrounded by an equatorial flat disk possibly still accreting, and an outflowing wind.
Amber Consortium
Benisty Myriam
Malbet Fabian
Tatulli Eric
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