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Fast shells and X-ray emission in 30 Doradus: SNRs and superbubbles
Published online by Cambridge University Press: 19 July 2016
Abstract
We have mapped the kinematics of the ionized gas in 30 Dor, and find numerous examples of fast expanding shells. There is good correlation between the high-velocity material and the bright diffuse X-ray emission in 30 Dor. The fast shells are probably supernova remnants, stellar wind-blown bubbles, or combinations of both.
- Type
- Large-Scale Structure and Kinematics
- Information
- Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 97 - 98
- Copyright
- Copyright © Kluwer 1991