Spectral analysis of (very) hot stars: Methods and results

Details Spectral analysis of (very) hot stars: Methods and results Spectral analysis of (very) hot stars: Methods and results

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218...33k&link_type=abstract

In ESA Fourth European IUE Conf. p 33-41 (SEE N84-35135 24-88)

Astronomy and Astrophysics

Astronomy

5

B Stars, O Stars, Planetary Nebulae, Spectrum Analysis, Stellar Spectra, Hertzsprung-Russell Diagram, Photosphere, Stellar Atmospheres, Stellar Evolution, Ultraviolet Astronomy

Scientific paper

Combined UV and visual quantitative spectral analysis of hot stars is summarized. The photospheres of very hot stars, the HR diagram of massive O stars, the atmospheres of subluminous OB stars, the atmospheres of the central stars of planetary nebulae, and the evolution of central stars of planetary nebulae and subluminous O and B stars were studied.

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