NASA NTRS · 19810017401
Highly-evolved stars
Abstract
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.
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Heap, S. R.. 1981-01-01. Highly-evolved stars. https://ntrs.nasa.gov/citations/19810017401
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