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• W2004488071 abstract "Far Ultraviolet Spectroscopic Explorer observations are presented for WD 0621-376, a DA white dwarf star in the local interstellar medium (LISM) at a distance of about 78 pc. The data have a signal-to-noise ratio of ∼20-40 per 20 km s-1 resolution element and cover the wavelength range 905-1187 Å. LISM absorption is detected in the lines of D I, C II, C II*, C III, N I, N II, N III, O I, Ar I, and Fe II. This sight line is partially ionized, with an ionized nitrogen fraction of greater than 0.23. We determine the ratio D/O = × 10-2 (2 σ). Assuming a standard interstellar oxygen abundance, we derive D/H ≈ 1.3 × 10-5. Using the value of N(H I) derived from Extreme Ultraviolet Explorer data gives a similar D/H ratio. The D I/N I ratio is × 10-1 (2 σ)." @default.
• W2004488071 created "2016-06-24" @default.
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• W2004488071 date "2002-05-01" @default.
• W2004488071 modified "2023-10-10" @default.
• W2004488071 title "Deuterium Abundance toward WD 0621−376: Results from the FUSE Mission" @default.
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• W2004488071 doi "https://doi.org/10.1086/339129" @default.
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