Abstract
We describe the evolution of the carbon dust shells around Very Late Thermal Pulse (VLTP) objects as seen at infrared wavelengths. This includes a 20-year overview of the evolution of the dust around Sakurai's object (to which Olivier made a seminal contribution) and FG Sge. VLTPs may occur during the endpoint of as many as 25% of solar mass stars, and may therefore provide a glimpse of the possible fate of the Sun.
| 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 | 281-286 |
| Number of pages | 6 |
| 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.