Ultraviolet carbon lines in the spectrum of the white dwarf BPM 11668.
Bibcode: 1983A&A...128..258W
Wegner, G.
United States
Abstract
The southern hemisphere DC white dwarf BPM 11668 has been found to show strong ultraviolet lines of neutral carbon using observations from the IUE satellite. This star seems typical of the growing number of DC white dwarfs found to be of this type and appears to have a carbon abundance near C:He = 10-5 with Teff = 8500K.
1983
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Astronomy and Astrophysics
IUE
10