The presence of carbon in DZ star atmospheres.
Bibcode: 1989A&A...210..311W
Koester, D.; Weidemann, V.
Germany, United States
Abstract
A recently obtained SWP spectrum of the DZ star L 119-34 is presented. The spectrum clearly shows the presence of C I lines. This result suggests that carbon is always present in cool helium-rich white dwarf atmospheres, independent of optically based spectral classification.
1989
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Astronomy and Astrophysics
IUE
9