Do stars of all masses acquire most of their mass via gravitational collapse of a single dense core?
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- Do stars of all masses acquire most of their mass via gravitational collapse of a single dense core?
- How are the properties of a star or binary determined by the properties of the medium from which it forms?
- How does the gas that goes into a protostar lose its magnetic flux and
angular momentum ? - How do massive stars form in the face of intense radiation pressure?
- What are the properties of the protostellar disks, jets, and outflows associated with young stellar objects (YSOs), and what governs their dynamical evolution?
- The macrophysics of star formation deals with the formation of systems of stars, ranging from clusters to galaxies.
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