Ultraviolet carbon lines in the spectrum of the white dwarf BPM 11668

Details Ultraviolet carbon lines in the spectrum of the white dwarf BPM 11668 Ultraviolet carbon lines in the spectrum of the white dwarf BPM 11668

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...128..258w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 128, no. 1, Nov. 1983, p. 258, 259.

Astronomy and Astrophysics

Astrophysics

8

Carbon, Stellar Atmospheres, Stellar Spectra, Ultraviolet Spectra, White Dwarf Stars, Iue, Line Spectra, Lyman Alpha Radiation, Southern Sky

Scientific paper

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.

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