Abstract
We perform radiation hydrodynamic simulations to study how very massive stars recover from giant eruptions. The post eruption star experience strong mass loss due to strong winds, driven by radial pulsations in the star's interior, that operate by the κ-mechanism. The mass loss history obtained in our simulations resembles η Car's history.
| Original language | English (US) |
|---|---|
| Title of host publication | The Physics of Evolved Stars |
| Subtitle of host publication | A Conference Dedicated to the Memory of Olivier Chesneau |
| Editors | F. Millour, T. Lanz, E. Lagadec |
| Publisher | EDP Sciences |
| Pages | 275-277 |
| Number of pages | 3 |
| ISBN (Electronic) | 9782759819072 |
| DOIs | |
| State | Published - Dec 1 2015 |
| Event | Physics of Evolved Stars Conference 2015 - Nice, France Duration: Jun 8 2015 → Jun 12 2015 |
Publication series
| Name | EAS Publications Series |
|---|---|
| Volume | 71-72 |
| ISSN (Print) | 1633-4760 |
| ISSN (Electronic) | 1638-1963 |
Other
| Other | Physics of Evolved Stars Conference 2015 |
|---|---|
| Country/Territory | France |
| City | Nice |
| Period | 6/8/15 → 6/12/15 |
Bibliographical note
Publisher Copyright:© 2015 EAS, EDP Sciences.
Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.