Model atmospheres and quantitative spectroscopy of central stars of planetary nebulae.
Modern quantitative spectroscopy of hot stars has two aspects: the analysis of spectral lines formed (1) in the hydrostatic photospheres and (2) in the supersonically expanding winds. Both aspects are covered by this paper.
- Pub Date:
- Planetary Nebulae: Central Stars;
- Central Stars: Stellar Models;
- Central Stars: Stellar Atmospheres;
- Central Stars: Spectroscopy;
- Central Stars: Stellar Evolution