| Download | - View final version: X-ray and radio emission from colliding stellar winds (PDF, 59.7 MiB)
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| DOI | Resolve DOI: https://doi.org/10.48550/arXiv.astro-ph/0409746 |
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| Author | Search for: Pittard, J. M.; Search for: Dougherty, S. M.1; Search for: Coker, R. F.; Search for: Corcoran, M. F. |
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| Affiliation | - National Research Council of Canada. NRC Herzberg Institute of Astrophysics
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| Format | Text, Article |
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| Conference | X-Ray and Radio Connections, 3-6 February 2004, Santa Fe, New Mexico, USA |
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| Subject | astrophysics |
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| Abstract | The collision of the hypersonic winds in early-type binaries produces shock heated gas, which radiates thermal X-ray emission, and relativistic electrons, which emit nonthermal radio emission. We review our current understanding of the emission in these spectral regions and discuss models which have been developed for the interpretation of this emission. Physical processes which affect the resulting emission are reviewed and ideas for the future are noted |
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| Publication date | 2004-09-30 |
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| Publisher | Cornell University |
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| Language | English |
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| Peer reviewed | No |
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| NPARC number | 9723302 |
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| Export citation | Export as RIS |
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| Report a correction | Report a correction (opens in a new tab) |
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| Record identifier | 6e8ffffc-31ee-467f-a1d8-8f4ebe06b39a |
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| Record created | 2009-07-17 |
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| Record modified | 2023-10-10 |
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