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Home > Art, Film & Photography > High Velocity Clouds: Interstellar Cloud, Magellanic Stream, Smith's Cloud, Hvc 127-41-330, Leo Ring
High Velocity Clouds: Interstellar Cloud, Magellanic Stream, Smith's Cloud, Hvc 127-41-330, Leo Ring

High Velocity Clouds: Interstellar Cloud, Magellanic Stream, Smith's Cloud, Hvc 127-41-330, Leo Ring


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About the Book

Chapters: Interstellar Cloud, Magellanic Stream, Smith's Cloud, Hvc 127-41-330, Leo Ring. Source: Wikipedia. Pages: 22. Not illustrated. Free updates online. Purchase includes a free trial membership in the publisher's book club where you can select from more than a million books without charge. Excerpt: The Magellanic Stream is a high-velocity cloud of gas connecting the Large and the Small Magellanic Clouds. It came into existence by a near-collision of both galaxies some 2.5 billion years ago. In 1965, anomalous velocity gas clouds were found in the region of the Magellanic Clouds. The gas stretches for at least 180 degrees across the sky. This corresponds to 180 kpc (600,000 ly) at an approximate distance of 55 kpc (180,000 ly). The gas is very collimated and polar with respect to the Milky Way. The velocity range is huge (from -400 to 400 km s in reference to Local Standard of Rest). Velocity patterns do not follow the rest of the Milky Way. So it was determined to be a classic High velocity cloud. But the gas was not mapped, and the connection to the two Magellanic Clouds was not made. The Magellanic Stream as such was discovered as a Neutral Hydrogen (HI) gas feature near the Magellanic Clouds by Wannier


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Product Details
  • ISBN-13: 9781158397273
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 152 mm
  • Sub Title: Interstellar Cloud, Magellanic Stream, Smith's Cloud, Hvc 127-41-330, Leo Ring
  • Width: 229 mm
  • ISBN-10: 1158397275
  • Publisher Date: 15 Sep 2010
  • Binding: Paperback
  • Spine Width: 1 mm
  • Weight: 50 gr


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