Dynamical ejections of stars due to an accelerating gas filament
Observations of the Orion A integral shaped filament (ISF) have shown indications of an oscillatory motion of the gas filament. This evidence is based on both thewave-likemorphology of the filament and the kinematics of the gas and stars, where the characteristic velocities of the stars require a dy...
| Main Authors: | , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
Oxford University Press
2017
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