Large Hot Subdwarfs and Extreme Horizontal Branch Stars

Details Large Hot Subdwarfs and Extreme Horizontal Branch Stars Large Hot Subdwarfs and Extreme Horizontal Branch Stars

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke1851s&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 1851. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Stellar Models And Concepts

Scientific paper

The hot subdwarf stars were first identified by their extremely blue colors in early field and cluster color-select photometric surveys (Humason and Zwicky 1947). Spectroscopic studies soon followed (Münch 1958, Greenstein 1965). From the cluster studies, it was quickly recognized that hot subdwarfs must have lower luminosities than main sequence stars of the same blue color, i.e. O and B stars, ...

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