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Dust-formation episode of the long-period WC+O binary WR 137: direct imaging with HST-NICMOS2
Published online by Cambridge University Press: 25 May 2016
Abstract
We have resolved, for the first time in any WR+OB system, IR-emitting dust in the close environment of the long-period binary WR 137. The dust emission occurs in a few clumps within about 0″.5 of the star, as well as in a jet-like structure with total extension of about 0″.25.
- Type
- Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
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- Copyright © Astronomical Society of the Pacific 1999