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The Metallicity and Dust Content of HVC287+22+240: Evidence for a Magellanic Clouds Origin
Published online by Cambridge University Press: 25 May 2016
Extract
We present evidence that the properties of the high-velocity cloud catalogued as #187 by Wakker & van Woerden (1991) (HVC287+22+240) can be explained if it is part of a leading arm counterpart of the Magellanic Stream, and we use this to argue that the HVC originated in the Magellanic Clouds after a tidal interaction.
- Type
- Part 7. Tidal Interactions
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 506 - 507
- Copyright
- Copyright © Astronomical Society of the Pacific 1999