Spectroscopic analysis of BPS CS 22940-0009: connecting evolved helium stars
arXiv:2208.07720 · doi:10.1093/mnras/stac2305
Abstract
BPS CS 22940-0009 is a helium-rich B-star that shares characteristics with both helium-rich B subdwarfs and extreme helium stars. The optical spectrum of BPS CS 22940-0009 has been analysed from SALT observations. The atmospheric parameters were found to be K, , , , , although further improvement to the helium line fits would be desirable. This places the star as a link between the He-sdB and EHe populations in - space. The abundance profile shows enrichment of N from CNO-processing, and C from burning. Depletion of Al, Si, S and a low upper limit for Fe show the star to be intrinsically metal-poor. The results are consistent with BPS CS 22940-0009 having formed from the merger of two helium white dwarfs and currently evolving toward the helium main sequence.
16 pages, 8 figures, to be published in Monthly Notices of the Royal Astronomical Society
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