Spectral analysis of the hottest known helium-rich white dwarf: KPD 0005+5106

Details Spectral analysis of the hottest known helium-rich white dwarf: KPD 0005+5106 Spectral analysis of the hottest known helium-rich white dwarf: KPD 0005+5106

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...284..907w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 284, no. 3, p. 907-918

Astronomy and Astrophysics

Astrophysics

36

Abundance, Helium, Spectrum Analysis, Stellar Atmospheres, Stellar Evolution, Ultraviolet Spectra, Visible Spectrum, White Dwarf Stars, X Ray Spectra, Atmospheric Models, Faint Object Camera, Hubble Space Telescope, Local Thermodynamic Equilibrium, Position Sensing, Proportional Counters, Rosat Mission, Spectrographs

Scientific paper

We present a non-Local Thermodynamic Equilibrium (LTE) model atmosphere
analysis of the helium-rich white dwarf KPD 0005+5106. The analysis is
based on optical spectra obtained at the Calar Alto 3.5 m telescope,
ultraviolet observations retrieved from the Hubble Space Telescope data
archive, and X-ray data recorded during the ROSAT all-sky survey.

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