Conference item icon

Conference item

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 ...

Expand abstract
Publication status:
Published

Actions


Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Theoretical Physics
Role:
Author
Journal:
COOL STARS, STELLAR SYSTEMS AND THE SUN, PROCEEDINGS
Volume:
223
Pages:
351-358
Publication date:
2001-01-01
Event title:
11th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Source identifiers:
26642
ISBN:
1583810560
Keywords:
Pubs id:
pubs:26642
UUID:
uuid:6550556c-3e5c-452a-b62c-b6571d955264
Local pid:
pubs:26642
Deposit date:
2012-12-19

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP