Next:
Hydrostatic Balance
Up:
Star Formation
1
Previous:
Galactic Shock
 
Contents
Local Star Formation Process
Subsections
Hydrostatic Balance
Problem 1
Problem 2
Bonnor-Ebert Mass
Equilibria of Cylindrical Cloud
Virial Analysis
Magnatohydrostatic Clouds
Subcritical Cloud vs Supercritical Cloud
Ambipolar Diffusion
Ionization Rate
Ambipolar Diffusion
Dynamical Collapse
Inside-out Collapse Solution
Protostellar Evolution of Supercritical Clouds
Accretion Rate
Problem
Outflow
Magneto-driven Model
Problem
Angular Momentum Transfer
Centrifugal Radius
Entrainment Model
Evolution to Star
Isothermal Phase
First Core
Second Collapse
Second Core
Example of Numerical Simulation
Evolution in the H-R diagram
Main Accretion Phase
Before Deuterium Ignition
After Deuterium Ignition
Premain-sequence Evolution
Kohji Tomisaka 2007-07-08