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- W2582145791 abstract "After a brief summary of observational information on gas with high and intermediate velocities, the objections against several possible origins for these phenomena are reviewed. The best hypothesis appears to be an intergalactic origin, near the Local Group. The intergalactic density required if the observed high-velocity flow is a continuing phenomenon is estimated at 10 to 100 × 10 -29 g cm -3 , depending on the z -distance of the intergalactic matter at the time of its deceleration by galactic gas, and on the importance of cosmic rays in this deceleration. The effects of the observed inflow of gas on galactic dynamics may be of great significance." @default.
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- W2582145791 date "1967-01-01" @default.
- W2582145791 modified "2023-09-25" @default.
- W2582145791 title "Possible interpretations of the high-velocity gas" @default.
- W2582145791 cites W2024191212 @default.
- W2582145791 doi "https://doi.org/10.1017/s007418090010107x" @default.
- W2582145791 hasPublicationYear "1967" @default.
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