# VLTI/AMBER unveils a possible dusty pinwheel nebula in WR118

@article{Millour2009VLTIAMBERUA,
title={VLTI/AMBER unveils a possible dusty pinwheel nebula in WR118},
author={F. Millour and Thomas Driebe and Olivier Chesneau and Jose H Groh and K. H. Hofmann and Koji Murakawa and Keiichi Ohnaka and Dieter Schertl and Gerd Weigelt},
journal={Astronomy and Astrophysics},
year={2009},
volume={506}
}
Most Wolf-Rayet stars (WR) of WC9 sub-type exhibit a dusty circumstellar envelope, but it is still a matter of debate how dust can form in their harsh environment. In a few cases, a pinwheel-like structure of the dusty envelope has been detected. Therefore, it has been suggested that dust formation in all dusty WR stars might be linked to colliding winds in a binary system. We probed the innermost region of the circumstellar dust shell of the deeply embedded WR star WR 118. We carried out…
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