A triple protostar system formed via fragmentation of a gravitationally unstable disk
Binary and multiple star systems are a frequent outcome of the star formation process1;2, and as a result, almost half of all sun-like stars have at least one companion star3. Theoretical studies indicate that there are two main pathways that can operate concurrently to form binary/multiple star sys...
Main Authors: | , , , , , , , , , , , |
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Language: | en |
Published: |
NATURE PUBLISHING GROUP
2016
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Online Access: | http://hdl.handle.net/10150/621528 http://arizona.openrepository.com/arizona/handle/10150/621528 |