The Helium Content and Evolution of Subdwarf O-Stars

Details The Helium Content and Evolution of Subdwarf O-Stars The Helium Content and Evolution of Subdwarf O-Stars

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981msngr..24....7h&link_type=abstract

The Messenger, No.24, P. 7, 1981

Mathematics

Logic

10

Scientific paper

Subdwarf 0 stars are faint blue stars that have luminosities 3- 8 magnitudes below the main sequence. In the Hertzsprung-Russell diagram they occupy a region intermediate between normal dwarfs and hot white dwarfs. Phenomenologically they appear as an extension 01 the horizontal branch towards very high temperatures (TeH > 35000 K). The link between the two classes form the subdwarf B stars.

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