The effect of convection on pulsational stability
| dc.creator | Houdek, G. | |
| dc.date | 2008-10-29 | |
| dc.date.accessioned | 2026-07-07T10:13:53Z | |
| dc.date.available | 2026-07-07T10:13:53Z | |
| dc.description | A review on the current state of mode physics in classical pulsators is presented. Two, currently in use, time-dependent convection models are compared and their applications on mode stability are discussed with particular emphasis on the location of the Delta Scuti instability strip. | |
| dc.description | Accepted for publication in CoAst (invited paper), 9 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/0810.5228 | |
| dc.identifier | http://arxiv.org/abs/0810.5228 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/172687 | |
| dc.subject | Astrophysics | |
| dc.title | The effect of convection on pulsational stability | |
| dc.type | text |