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high-velocity cloud

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high-velocity cloud [′hī və′läs·əd·ē ′klau̇d]
(astronomy)
A rapidly moving interstellar cloud with a radial velocity greater than about 12 miles (20 kilometers) per second, consisting primarily of neutral atomic hydrogen, observed in the ultraviolet.


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The Andromeda finding strengthens the case that the high-velocity clouds surrounding the Milky Way include remnant gas from the galaxy's origin, says Thilker.
Afterward, a slower-moving yet still high-velocity cloud of dust, debris and molten material swept over North America, ``adding more insult,'' Schultz said.
Astronomers had assumed the body was a so-called high-velocity cloud, a type of fast-moving mass of atomic hydrogen commonly found far from the galaxy.
 
 
 
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