Spectroscopic and photometric observations of white dwarfs

Details Spectroscopic and photometric observations of white dwarfs Spectroscopic and photometric observations of white dwarfs

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...108..406k&link_type=abstract

Astronomy and Astrophysics, vol. 108, no. 2, Apr. 1982, p. 406-411.

Astronomy and Astrophysics

Astrophysics

15

Astronomical Spectroscopy, Image Dissector Tubes, Stellar Spectrophotometry, Ubv Spectra, Visible Spectrum, White Dwarf Stars, Absorption Spectra, Abundance, Carbon Stars, Fraunhofer Lines, H Alpha Line, Helium, Neutral Atoms, Spectral Line Width, Stellar Spectra, Ultraviolet Photometry

Scientific paper

Image Dissector Scanner (IDS) observations obtained at the ESO 3.6 m
telescope, and uvby colors are reported for a variety of white dwarfs of
spectral types DB, DC, C2, and DA as well as some white dwarf
candidates. G 268-40 is shown to be the third C2 star with lines of
neutral carbon in the visible spectrum.

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