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• W1539199891 abstract "Abstract Previous published absorption line studies performed at ultraviolet and visual wavelengths are combined with new ultraviolet data in order to map out the distribution of HI within 150 pc of the Sun. Newly presented data for distances less than 50 pc further support the local cloud model as presented by Bruhweiler (1982). The Sun is embedded, near the edge of a diffuse cloud with total column density of 2 x 10 19 cm -2 . Most observed directions within 50 pc away from the cloud body reveal trace amounts of gas (N)HI) ~ 10 18 cm -2 ) presumably arising in the outer skin of the local cloud. At greater distances (50 ≲ d ≲ 150 pc) most directions show significant absorption with N(HI)>10 19 cm -2 . Two directions, one toward the northern galactic pole (NGP), the other toward β CMa exhibit unusually low HI column densities out to distances of 150-200 pc. However, substantial amounts of gas, N(HI) > 10 19 cm -2 , are seen toward the NGP at greater distances. The implications of these results on astronomy at wavelengths shortward of 912Å are discussed." @default.
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• W1539199891 date "1984-01-01" @default.
• W1539199891 modified "2023-10-18" @default.
• W1539199891 title "Absorption Line Studies and the Distribution of Neutral Gas in the Local Interstellar Medium" @default.
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• W1539199891 doi "https://doi.org/10.1017/s0252921100097955" @default.
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