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MT Thermometer:
0.46
Magnetic Fields or Turbulence:
Which is the critical factor for the formation of stars and planetary disks?
February 6(Tue)-9(Fri), 2018
National Tsing Hua University, Hsinchu, Taiwan

Invited Presentation

Magnetically regulated collapse in the B335 protostar ? ALMA observations and MHD models

Author(s): Anaëlle Maury (CEA) Maud Galametz (CEA) et al.

Presenter: Anaëlle Maury (CEA Astrophysics department, Paris-Saclay University)

Recent observational and theoretical results highlight the role of magnetic braking for several long-standing problems in astronomy such as the angular momentum problem, and the formation of stellar binaries and disks.
We carried out an SMA survey of the polarized dust emission in a sample of low-mass Class 0 protostars, which main results I will present. I will then focus on the B335 protostar for which we obtained follow-up ALMA observations. We have confronted our observational constraints in B335 with realistic outputs from non-ideal MHD simulations of core collapse.
I will present our first results attempting to characterize the magnetic field roles in this young protostar, using ALMA observations and MHD simulations.

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