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The Aftermaths of the SMC/LMC Encounter
Published online by Cambridge University Press: 25 May 2016
Abstract
We present structural and kinematic evidence pointing to a gravitational interaction between the two Magellanic Clouds. We discuss, in particular, the results of our kinematic survey of carbon stars in the periphery of the LMC. Stars with peculiar velocities, in the LMC southwest, are identified as part of debris left on the SMC orbit around the LMC.
- Type
- Part 7. Tidal Interactions
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 487 - 491
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
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