Abstract
As part of an extended study of the surface abundances of extremely helium-rich hot subdwarfs, high-resolution optical échelle spectra of the three helium-rich subdwarf B stars LB 1766, SB 21 and BPS 22940–0009 are presented. Opacity-sampled line-blanketed model atmospheres have been used to derive atmospheric properties and surface abundances. All three stars are moderately metal-poor compared with the Sun ([Fe/H]≈−0.4). The first two stars are nitrogen-rich He-sdBs, while the third is a carbon-rich He-sdB. The surface composition and locus of single N-rich He-sdBs are currently best explained by the merger of two helium white dwarfs. C-rich He-sdBs require further investigation.
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N., N., Jeffery, C.S., Ahmad, A. et al. Abundance analyses of three helium-rich sdB stars. Astrophys Space Sci 329, 119–125 (2010). https://doi.org/10.1007/s10509-010-0334-x
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DOI: https://doi.org/10.1007/s10509-010-0334-x