Protostellar Disc and Outflow Formation in Low- and High-Mass Dense Core Collapse
Abstract
I will present the results of magnetised dense cores collapse 3D simulations including ambipolar diffusion with the adaptive-mesh-refinement code RAMSES. The numerical models cover a wide range of initial masses, form one to hundred solar masses, as well as the effect of initial rotation and/or turbulence. I will show how ambipolar diffusion acts on the formation of protostellar disks, which can subsequently launch collimated outflows. I will detail the properties of the disks and outlfows and the similarities between low and high-mass star formation.
- Publication:
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Star Formation from Cores to Clusters
- Pub Date:
- June 2017
- DOI:
- 10.5281/zenodo.808562
- Bibcode:
- 2017sfcc.confE...9C
- Keywords:
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- Zenodo community starformation2017