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Studies of cool giant stars using GHRS spectra

Abstract:

Observations with the GHRS have made a considerable impact on the study of cool stars. Observations with the International Ultraviolet Explorer established the overall nature of the UV spectra of cool evolved stars, but only strong sources could be observed at high resolution and measurements of line widths were impeded by the lower signal-to-noise, The greater sensitivity of the GHRS has allowed many more emission lines to be observed, in particular, weak lines of C IV and fluorescent lines ...

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Publication status:
Published

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Institution:
University of Oxford
Department:
Oxford, MPLS, Physics, Theoretical Physics
Role:
Author
Volume:
223
Pages:
351-358
Publication date:
2001-01-01
URN:
uuid:6550556c-3e5c-452a-b62c-b6571d955264
Source identifiers:
26642
Local pid:
pubs:26642
ISBN:
1-58381-056-0

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