| |
 |
| Paper: |
HD 52961 - A pulsating post-AGB-star with extremely low metal content |
| Volume: |
11, Confrontation Between Stellar Pulsation and Evolution |
| Page: |
125 |
| Authors: |
Waelkens, C.; Van Winckel, H.; Bogaert, E. |
| Abstract: |
In an study of IRAS point sources with optical counterparts, HD 52961 has been shown to be one of the most metal-poor stars in the Galaxy. It is a pulsating star with a period of 72 days. Its IR excess and the CNO enhancements indicate that it is a post-AGB (asymptotic giant branch) star. |
|
|
|
|
|
