Astrophysics (Index)About

Magellanic Stream

(series of high-velocity clouds associated with the Magellanic Clouds)

The Magellanic Stream is a high-velocity cloud (HVC) or series of HVCs leading away from the Magellanic clouds along a line across the celestial sphere. In our view, it extends 180 degrees across the sky. They are gas clouds, but a young stellar cluster has been identified within them. The initially discovered clouds tail the movement of the Magellanic Clouds in their orbit around the Milky Way, but the stream is now observed to extend forward along this trajectory as well. They are presumed to have formed from tidal force on the Magellanic Clouds from the Milky Way, shaped by hydrodynamic forces within the Milky Way galactic halo.


(cloud,Milky Way)
Further reading:
http://en.wikipedia.org/wiki/Magellanic_Stream
RedshiftParsecs
/Distance
Lightyears
/Lookback Years
  
~055kpc179klyMagellanic Stream
Coordinates:Magellanic Stream
0032-30

Referenced by pages:
high-velocity cloud (HVC)

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