Now showing items 1-2 of 2
Three case studies in spectroscopic mode identification of non-radially pulsating stars
(University of Canterbury. Physics and Astronomy, 2011)
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 ...
Spectroscopic mode identification in a sample of non-radially pulsating stars
(University of Canterbury. Physics and Astronomy, 2008)
This thesis has analysed spectroscopic data for three stars in detail, the β Cephei star V2052 Ophiuchus, the γ Doradus star QW Puppis and the γ Doradus candidate star HD139095. Twelve other candidate γ Doradus stars have ...