Non-LTE model for the wind of the NGC 6543 central star
Abstract
We present non-LTE models of the wind for the central star in NGC 6543. The models suggest that the star is hydrogen-rich. The iron composition is solar, which, in turn, suggests that the hot X-ray emitting gas is of nebular origin.
- Publication:
-
Planetary Nebulae in our Galaxy and Beyond
- Pub Date:
- 2006
- DOI:
- 10.1017/S1743921306003449
- Bibcode:
- 2006IAUS..234..401G