Paolo Padoan
0000-0002-5055-5800
94 papers found
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Turbulence-Induced Relative Velocity of Dust Particles. Ii. The Bidisperse Case
Turbulence-Induced Relative Velocity of Dust Particles. I. Identical Particles
Zooming in on the Formation of Protoplanetary Disks
A Simple Law of Star Formation
ERRATUM: “AMBIPOLAR DRIFT HEATING IN TURBULENT MOLECULAR CLOUDS” (2000, ApJ, 540, 332)
The Two States of Star-Forming Clouds
The Observable Prestellar Phase of the Initial Mass Function
Turbulent Clustering of Protoplanetary Dust and Planetesimal Formation
Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence
Accuracy of core mass estimates in simulated observations of dust emission
Population Iii Stars From Turbulent Fragmentation at Redshift ∼11
Mass and Magnetic Distributions in Self-Gravitating Super-Alfvénic Turbulence With Adaptive Mesh Refinement
The Star Formation Rate of Supersonic Magnetohydrodynamic Turbulence
Relative velocity of inertial particles in turbulent flows
Magnetic Fields in Molecular Clouds
Theory of the Star Formation Rate
The IMF of stellar clusters: effects of accretion and feedback
MHD turbulence in star-forming clouds
The Power Spectrum of Turbulence in Ngc 1333: Outflows or Large-Scale Driving?
The Super-Alfvénic Model of Molecular Clouds: Predictions for Mass-To-Flux and Turbulent-To-Magnetic Energy Ratios
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