Wolf-Rayet stars - A normal developmental phase of the most massive stars

Details Wolf-Rayet stars - A normal developmental phase of the most massive stars Wolf-Rayet stars - A normal developmental phase of the most massive stars

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989s%26w....28...81l&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 28, Feb. 1989, p. 81-88. In German.

Astronomy and Astrophysics

Astronomy

Astrometry, Stellar Evolution, Supermassive Stars, Wolf-Rayet Stars, Abundance, Blue Stars, Classifications, Emission Spectra, Line Spectra, Nuclear Fusion, Star Formation, Stellar Envelopes, Stellar Luminosity, Stellar Magnitude, Supernovae

Scientific paper

Observational data and theoretical models for WR stars are examined in a general review. The most striking features of the WR spectrum are discussed, with a focus on the role of the gas envelope, and consideration is given to the interpretation of surface abundances, the inner structure of the WR star, scenarios proposed to explain the origin of WR stars, WR-star evolution, the relationship between WR stars and SN, and the more general implications of WR-star studies. Diagrams, graphs, and sample images are provided.

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