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Pressure-regulated, Feedback-modulated Star Formation in Disk Galaxies
Eve C. Ostriker
,
Chang Goo Kim
Astrophysical Sciences
Princeton Center for Theoretical Science (PCTS)
Princeton Institute for Computational Science and Engineering
Research output
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Contribution to journal
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Article
›
peer-review
62
Scopus citations
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Keyphrases
Star Formation
100%
Star Formation Rate
100%
Disk Galaxies
100%
Interstellar Medium
66%
Physical State
50%
ISM
33%
Total Pressure
33%
Numerical Simulation
16%
Magnetohydrodynamic Simulation
16%
Velocity Dispersion
16%
Surface Density
16%
Mid-plane
16%
High Pressure
16%
Massive Stars
16%
Star-forming
16%
Radiative Cooling
16%
Supernovae
16%
Thermal Phase
16%
Galactic Disks
16%
Quasi-steady State
16%
Simulation Runs
16%
Computational Framework
16%
Gravitational Field
16%
Turbulent Dissipation
16%
Dark Matter Density
16%
Medium Weight
16%
Medium Gas
16%
Feedback Energy
16%
Medium Velocity
16%
Physics
Star Formation
100%
Star Formation Rate
100%
Disk Galaxy
100%
Interstellar Matter
66%
Magnetohydrodynamic Simulation
16%
Massive Star
16%
Supernovae
16%
Gravitational Field
16%
Quasi-Steady State
16%
Stellar Radiation
16%
Dark Matter Density
16%