Article contents
Driving g-mode Pulsations in γ Doradus Variables
Published online by Cambridge University Press: 12 April 2016
Abstract
We suggest that the modulation of radiative flux by convection at the base of a deep envelope convection zone during the pulsation cycle is responsible for driving high-order g modes with periods 0.4 to 3 d observed in γ Doradus variables.
- Type
- Part 6. Variables Close to the Main Sequence
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2000
References
- 1
- Cited by