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NLTE Analysis of Extremely Helium Rich Subdwarf O-Stars
1993The NLTE analyses of four extremely helium rich sdO stars are presented. Effective temperatures, gravities and the abundances of H, He, C, N, O, Ne, Mg and Si have been determined. It is found that three of the programme stars have very similar parameters. The positions of these stars in the (T eff,log g) diagram indicate, that they are post-EHB stars.
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A spectroscopic and photometric investigation of the extreme helium-rich star HD 168476
1979Spectra were obtained from several sources for a fine abundance analysis of the extreme helium-rich star HD 168476. The atmospheric parameters are found using theoretical models and abundances determined for the ions identified in the spectra.
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Pulsation Stability of Helium-Rich Subdwarf B Stars
Astrophysics and Space Science, 2004J -E Solheim, C S Jeffery, R Østensen
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NLTE Spectral Analysis of the Intermediate Helium-Rich Subdwarf B Star CPD−20°1123
Monthly Notices of the Royal Astronomical Society, 2020Lisa Löbling
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Abundance Analyses of Three Helium-Rich sdB Stars
Astrophysics and Space Science, 2010Timur Şahin, C S Jeffery
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New Helium Spectrum Variable and a New Helium-Rich Star.
Publications of the Astronomical Society of the Pacific, 1975N R Walborn
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Outbursts of Luminous Blue Variable Stars From Variations in the Helium Opacity
Nature, 2018Lars Bildsten +2 more
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Discovery of Pulsation in a Helium-Rich Subdwarf B Star
Astronomy and Astrophysics, 2005C S Jeffery
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Physical Parameters of Helium-Rich Subdwarf B Stars From Medium Resolution Optical Spectroscopy
Astronomy and Astrophysics, 2003C S Jeffery
exaly

