No CrossRef data available.
Article contents
Dust formation in, and the structure of wolf-rayet stellar winds
Published online by Cambridge University Press: 04 August 2017
Abstract
An infrared photometric survey of all 40 known galactic WC7-10 stars shows that around most of them hot amorphous carbon is condensing continuously at distances of about 8500 R⊙, well within the ionized stellar winds around these stars. Typical dust production rates are of the order of 10−7 M⊙/yr.
- Type
- Mass Loss from Hot Stars
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 455 - 456
- Copyright
- Copyright © Reidel 1987