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- W1984797534 abstract "Abstract Since HI, OI, and DI have nearly the same ionization potential, the deuterium-to-oxygen ratio (D/O) is an important tracer of the D/H ratio and its putative spatial variations. D/O is indeed very sensitive to astration, both because of deuterium destruction and oxygen production. Here, we present DI, OI, and NI interstellar column density measurements performed with the Far Ultraviolet Spectroscopic Explorer (FUSE) on eight nearby lines of sight. The first results of this survey show that D/O is a better D/H proxy than D/N, and that D/O is constant in the local interstellar medium. The mean value is D / O =3.81(±0.18)×10 −2 (1σ) . This result supports both D/H and O/H stability in the LISM." @default.
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- W1984797534 date "2002-10-01" @default.
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- W1984797534 title "The deuterium-to-oxygen ratio in the local interstellar medium from FUSE observations" @default.
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- W1984797534 doi "https://doi.org/10.1016/s0032-0633(02)00078-8" @default.
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