Studies of cool giant stars using GHRS spectra
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 lin...
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| Format: | Conference item |
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2001
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| _version_ | 1826276208269066240 |
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| author | Jordan, C McMurry, A |
| author_facet | Jordan, C McMurry, A |
| author_sort | Jordan, C |
| collection | OXFORD |
| description | 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 of Fe II, HZ and CO in a Tau (K5 III). These and other examples of how GHRS observations have led to improvements in spectroscopy and understanding cool giant atmospheres are discussed. |
| first_indexed | 2024-03-06T23:10:34Z |
| format | Conference item |
| id | oxford-uuid:6550556c-3e5c-452a-b62c-b6571d955264 |
| institution | University of Oxford |
| last_indexed | 2024-03-06T23:10:34Z |
| publishDate | 2001 |
| record_format | dspace |
| spelling | oxford-uuid:6550556c-3e5c-452a-b62c-b6571d9552642022-03-26T18:24:46ZStudies of cool giant stars using GHRS spectraConference itemhttp://purl.org/coar/resource_type/c_5794uuid:6550556c-3e5c-452a-b62c-b6571d955264Symplectic Elements at Oxford2001Jordan, CMcMurry, AObservations 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 of Fe II, HZ and CO in a Tau (K5 III). These and other examples of how GHRS observations have led to improvements in spectroscopy and understanding cool giant atmospheres are discussed. |
| spellingShingle | Jordan, C McMurry, A Studies of cool giant stars using GHRS spectra |
| title | Studies of cool giant stars using GHRS spectra |
| title_full | Studies of cool giant stars using GHRS spectra |
| title_fullStr | Studies of cool giant stars using GHRS spectra |
| title_full_unstemmed | Studies of cool giant stars using GHRS spectra |
| title_short | Studies of cool giant stars using GHRS spectra |
| title_sort | studies of cool giant stars using ghrs spectra |
| work_keys_str_mv | AT jordanc studiesofcoolgiantstarsusingghrsspectra AT mcmurrya studiesofcoolgiantstarsusingghrsspectra |