A further list and some properties of red degenerates. XI

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Abundance, Late Stars, Stellar Spectra, Subdwarf Stars, White Dwarf Stars, Carbon Stars, Line Spectra, Metals, Stellar Luminosity, Stellar Motions, Tables (Data)

Scientific paper

New multichannel SIT observations of 78 faint stars, including 51 new degenerates, are given. Helium and carbon stars, and one with a Zeeman triplet (magnetic field), are included. Red subluminous stars are distinguished by ultraviolet absorption but can be confused with red degenerates at the multichannel resolution. The sample includes a number of stars fainter than +15; properties of 25 such faint degenerates are tabulated. Deviations from a smooth interpolation formula show most red degenerates to be essentially line-free, i.e., to have extremely low metal abundance.

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