Fragmentation and disk formation in high-mass star formation: The ALMA view of G351.77-0.54 at 0.06" resolution
© ESO, 2017. Context. The fragmentation of high-mass gas clumps and the formation of the accompanying accretion disks lie at the heart of high-mass star formation research. Aims. We resolve the small-scale structure around the high-mass hot core G351.77-0.54 to investigate its disk and fragmentation...
| Main Authors: | , , , , , , |
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| Format: | Journal Article |
| Published: |
EDP Sciences
2017
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| Online Access: | http://hdl.handle.net/20.500.11937/68775 |