Paolo Padoan
0000-0002-5055-5800
94 papers found
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Synthetic observations of dust emission and polarisation of Galactic cold clumps
The CARMA-NRO Orion Survey: Core Emergence and Kinematics in the Orion A Cloud
The Probability Distribution of Density Fluctuations in Supersonic Turbulence
Expanding associations in the Vela-Puppis region
Inaccuracy of Spatial Derivatives in Riemann Solver Simulations of Supersonic Turbulence
The CARMA-NRO Orion Survey
Detailed Balance and Exact Results for Density Fluctuations in Supersonic Turbulence
The Stellar IMF from Isothermal MHD Turbulence
The magnetic field of molecular clouds
Supernova Driving. IV. The Star-formation Rate of Molecular Clouds
Supernova Driving. Iii. Synthetic Molecular Cloud Observations
Supernova Driving. Ii. Compressive Ratio in Molecular-Cloud Turbulence
Supernova Driving. I. The Origin of Molecular Cloud Turbulence
Protostellar accretion traced with chemistry
Turbulence-Induced Relative Velocity of Dust Particles V. Testing Previous Models
The Relative and Absolute Ages of Old Globular Clusters in the Lcdm Framework
Turbulence-Induced Relative Velocity of Dust Particles. Iv. The Collision Kernel
Infall-Driven Protostellar Accretion and the Solution to the Luminosity Problem
Turbulence-Induced Relative Velocity of Dust Particles. Iii. The Probability Distribution
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