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Highly-evolved stars
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Heap, S. R. |
| Copyright Year | 1981 |
| Description | The ways in which the IUE has proved useful in studying highly evolved stars are reviewed. The importance of high dispersion spectra for abundance analyses of the sd0 stars and for studies of the wind from the central star of NGC 6543 and the wind from the 0 type component of Vela X-1 is shown. Low dispersion spectra are used for absolute spectrophotometry of the dwarf nova, Ex Hya. Angular resolution is important for detecting and locating UV sources in globular clusters. |
| File Size | 827940 |
| Page Count | 20 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19810017401 |
| Archival Resource Key | ark:/13960/t9r25rt9w |
| Language | English |
| Publisher Date | 1981-01-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Stellar Spectra Stellar Winds Radio Astronomy Spaceborne Astronomy Binary Stars Iue Stellar Evolution Stellar Spectrophotometry Dwarf Stars Globular Clusters Ntrs Nasa Technical Reports ServerĀ (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Article |