Volume 504, Number 1, September II 2009
|Page(s)||115 - 125|
|Section||Interstellar and circumstellar matter|
|Published online||09 July 2009|
The close circumstellar environment of Betelgeuse*
Adaptive optics spectro-imaging in the near-IR with VLT/NACO
LESIA, Observatoire de Paris, CNRS UMR 8109, UPMC, Université Paris Diderot, 5 place Jules Janssen, 92195 Meudon, France e-mail: Pierre.Kervella@obspm.fr
2 Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
3 National Optical Astronomy Observatories, 950 North Cherry Avenue, Tucson, AZ 85719, USA
4 Physics and Astronomy Dept, University of Western Ontario, London ON N6A 3K7, Canada
5 SETI Institute, 515 North Whisman Road, Mountain View, CA 94043, USA
Accepted: 22 June 2009
Context. Betelgeuse is one the largest stars in the sky in terms of angular diameter. Structures on the stellar photosphere have been detected in the visible and near-infrared as well as a compact molecular environment called the MOLsphere. Mid-infrared observations have revealed the nature of some of the molecules in the MOLsphere, some being the precursor of dust.
Aims. Betelgeuse is an excellent candidate to understand the process of mass loss in red supergiants. Using diffraction-limited adaptive optics (AO) in the near-infrared, we probe the photosphere and close environment of Betelgeuse to study the wavelength dependence of its extension, and to search for asymmetries.
Methods. We obtained AO images with the VLT/NACO instrument, taking advantage of the “cube” mode of the CONICA camera to record separately a large number of short-exposure frames. This allowed us to adopt a “lucky imaging” approach for the data reduction, and obtain diffraction-limited images over the spectral range m in 10 narrow-band filters.
Results. In all filters, the photosphere of Betelgeuse appears partly resolved. We identify an asymmetric envelope around the star, with in particular a relatively bright “plume” extending in the southwestern quadrant up to a radius of approximately six times the photosphere. The CN molecule provides an excellent match to the 1.09 μm bandhead in absorption in front of the stellar photosphere, but the emission spectrum of the plume is more difficult to interpret.
Conclusions. Our AO images show that the envelope surrounding Betelgeuse has a complex and irregular structure. We propose that the southwestern plume is linked either to the presence of a convective hot spot on the photosphere, or to the rotation of the star.
Key words: stars: individual: Betelgeuse / stars: imaging / stars: supergiants / stars: circumstellar matter / methods: observational / techniques: high angular resolution
© ESO, 2009
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