The presence of carbon in DZ star atmospheres

Details The presence of carbon in DZ star atmospheres The presence of carbon in DZ star atmospheres

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...210..311w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 210, no. 1-2, Feb. 1989, p. 311, 312.

Astronomy and Astrophysics

Astrophysics

6

Abundance, Carbon, Stellar Atmospheres, Stellar Spectrophotometry, Ultraviolet Spectra, White Dwarf Stars, Iue, Metallicity, Resonance Lines, Spectral Energy Distribution

Scientific paper

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.

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