Star-formation (II)
14 Maio 2020, 14:00 • Israel Matute
Gravitational collapse of dense cores.
Gravitational collapse of cores - Virial Theorem
Jeans Mass/Radius equations and examples based on actual conditions for the collapsing clouds.
Bonnor-Ebert Mass
Fragmentation during collapse
Conditions for max. Fragmentation: Isothermal vs Adiabatic and discussion on what other important physical processes could be important but initially neglected, e.g. magnetic fields and rotation.
Discussed that more detailed models set a limit for max fragmentation on 0.01 M⊙.