Fragmentation and massive disk formation
Henrik Beuther
MPIA, Heidelberg, DE
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How do high-mass gas clumps fragment? And how do the most massive
disk-like structures form during this process? I will present results
from a new large program at NOEMA (formerly Plateau de Bure
Interferometer) resolving a large sample of high-mass star-forming
regions at mm wavelength around 0.3" resolution. This program
resolves the central cores and reveal the gas dynamics. These data
will be complemented with recent even higher resolution (< 0.1") data
from ALMA and the VLA toward two specific case studies.
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Suggested Session:
Disk Formation
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