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The winds and coronae of early-type stars
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Cassinelli, J. P. |
| Copyright Year | 1983 |
| Description | The properties of the winds of hot stars as derived from radio, ultraviolet and X-ray observations is presented. Special focus is given to observations that test line driven wind theory. In this theory the wind properties are determined by the stellar effective temperature and surface gravity, but not parameters that specify the mechanical or wave fluxes from the star. Alternate explanations of the X-ray emission from the early-type stars are discussed. Evidence is given for the presence of coronal zones at the base of the stellar winds. |
| File Size | 783136 |
| Page Count | 16 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19840005018 |
| Archival Resource Key | ark:/13960/t2j728t30 |
| Language | English |
| Publisher Date | 1983-11-01 |
| Access Restriction | Open |
| Subject Keyword | Solar Physics Stellar Winds Radio Astronomy Stellar Temperature Emission Spectra Wind Profiles Line Spectra X Ray Astronomy Early Stars Stellar Coronas Ultraviolet Astronomy Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |
