Paolo Padoan

Dartmouth College — United States

Physics and Astronomy · Physical Sciences

40h-index6.5kcitations151works4.32yr avg
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Research Topics

Astrophysics and Star Formation Studies(112), Stellar, planetary, and galactic studies(73), Astro and Planetary Science(42), Atmospheric Ozone and Climate(33), Solar and Space Plasma Dynamics(26)

Publications151 total

Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies
Monthly Notices of the Royal Astronomical Society·2025· 4 citedOpen Access
The formation of protoplanetary disks through pre-main-sequence Bondi–Hoyle accretion
Nature Astronomy·2025· 5 cited
Origin and evolution of angular momentum of class II disks
Astronomy and Astrophysics·2025· 6 citedOpen Access
Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies
arXiv (Cornell University)·2025· 1 citedOpen Access
Updated Kinematics of the Radcliffe Wave: Nonsynchronous, Dipole-like Vertical Oscillations
The Astrophysical Journal·2024· 4 citedOpen Access
The Formation of Protoplanetary Disks through Pre-Main Sequence Bondi-Hoyle Accretion
arXiv (Cornell University)·2024· 5 citedOpen Access
Origin and Evolution of Angular Momentum of Class II Disks
arXiv (Cornell University)·2024· 2 citedOpen Access
Evaporation ages: A new dating method for young star clusters
Astronomy and Astrophysics·2024· 7 citedOpen Access
Evaporation Ages: a New Dating Method for Young Star Clusters
arXiv (Cornell University)·2023Open Access
Will ALMA reveal the true core mass function of protoclusters?
Monthly Notices of the Royal Astronomical Society·2023· 9 citedOpen Access
CARMA-NRO Orion Survey: Unbiased Survey of Dense Cores and Core Mass Functions in Orion A
The Astrophysical Journal Supplement Series·2023· 14 citedOpen Access
Will ALMA Reveal the True Core Mass Function of Protoclusters?
arXiv (Cornell University)·2023Open Access
CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A
arXiv (Cornell University)·2022Open Access
Physical properties and real nature of massive clumps in the galaxy
Monthly Notices of the Royal Astronomical Society·2021· 1 citedOpen Access
The dynamical state of massive clumps
Monthly Notices of the Royal Astronomical Society·2021Open Access
From the CMF to the IMF: beyond the core-collapse model
Monthly Notices of the Royal Astronomical Society·2021· 44 citedOpen Access
Dust polarization studies on MHD simulations of molecular clouds: comparison of methods for the relative-orientation analysis
Springer Link (Chiba Institute of Technology)·2021· 3 cited
The CARMA-NRO Orion Survey—Data Release
Research Notes of the AAS·2021· 2 citedOpen Access
The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?
The Astrophysical Journal Letters·2021· 20 citedOpen Access
From the CMF to the IMF: Failure of the Core-Collapse Model
arXiv (Cornell University)·2020Open Access
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Frequent Co-authors

Åke Nordlund(25), M. Juvela(12), Alexei G. Kritsuk(8), Michael L. Norman(8), V.-M. Pelkonen(6), Liubin Pan(6), Raúl Jiménez(5), David C. Collins(4), Stanislav Boldyrev(4), Troels Haugbølle(4), John Bally(4), Alyssa Goodman(3), Hao Xu(3), Bernard J. T. Jones(2), Pak Shing Li(2), S. D. Ustyugov(2), Christoph Federrath(2), T. Cantat-Gaudin(2), C. Jordi(2), N. J. Wright(2)