Three case studies in spectroscopic mode identification of non-radially pulsating stars
Gravity modes present in gamma Doradus stars probe the deep stellar interiors and are thus of particular interest in asteroseismology. Mode identification will improve the knowledge of these stars considerably and allow an understanding of the issues with current pulsational models. The methods used...
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| Language: | en |
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University of Canterbury. Physics and Astronomy
2011
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| Online Access: | http://hdl.handle.net/10092/5395 |