PP
Paolo Padoan
astro-phastro-ph.GAastro-ph.SRphysics.flu-dynastro-ph.COastro-ph.EPnlin.CD
On Valency
published · living versionsW_tzpdnd69·v1 · currentpublished
Slow Massive-Star Formation and the O-Star ZAMS Deficit
with Samuel Shipkoff, Mark Gieles, Fabrice Martins
1 version
Preprints & journals
94 papers in the corpus · 1995–2026Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects2608.00441v1 · Dana Makarova, Dana Alina, Paolo Padoan et al.2026 · 0 citationsarXiv
Random gas motions inside sub-parsec scale supercritical filaments2604.04501v4 · Chao Zhang, Tie Liu, Mika Juvela et al.2026 · 5 citationsScience China Physics, Mechanics & Astronomy Volume 69, Issue 8: 289512 (2026)
Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales2602.06196v2 · Paolo Padoan, Mark Gieles2026 · 0 citationsarXiv
Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies2501.12138v3 · Mark Gieles, Paolo Padoan, Corinne Charbonnel et al.2025 · 18 citationsarXiv
The Formation of Protoplanetary Disks through Pre-Main Sequence Bondi-Hoyle Accretion2405.07334v2 · Paolo Padoan, Liubin Pan, Veli-Matti Pelkonen et al.2024 · 18 citationsarXiv
Origin and Evolution of Angular Momentum of Class II Disks2405.06520v2 · Veli-Matti Pelkonen, Paolo Padoan, Mika Juvela et al.2024 · 13 citationsA&A 694, A327 (2025)
Evaporation Ages: a New Dating Method for Young Star Clusters2311.08363v2 · V.-M. Pelkonen, N. Miret-Roig, P. Padoan2023 · 10 citationsarXiv
Will ALMA Reveal the True Core Mass Function of Protoclusters?2301.07398v2 · Paolo Padoan, Veli-Matti Pelkonen, Mika Juvela et al.2023 · 11 citationsarXiv
CARMA-NRO Orion Survey: unbiased survey of dense cores and core mass functions in Orion A2211.10215v2 · Hideaki Takemura, Fumitaka Nakamura, H'ector G. Arce et al.2022 · 16 citationsarXiv
The Dynamical State of Massive Clumps2111.08887v1 · Zu-Jia Lu, Veli-Matti Pelkonen, Mika Juvela et al.2021 · 0 citationsarXiv
Physical Properties and Real Nature of Massive Clumps in the Galaxy2108.08981v1 · Zu-Jia Lu, Veli-Matti Pelkonen, Mika Juvela et al.2021 · 1 citationarXiv
The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?2103.08527v1 · Hideaki Takemura, Fumitaka Nakamura, Shuo Kong et al.2021 · 22 citationsarXiv
From the CMF to the IMF: Beyond the Core-Collapse Model2008.02192v4 · V.-M. Pelkonen, P. Padoan (1, T. Haugb\olle et al.2020 · 52 citationsarXiv
The CARMA-NRO Orion Survey: Core Emergence and Kinematics in the Orion A Cloud1908.04488v1 · Shuo Kong, H'ector G. Arce, Anneila I. Sargent et al.2019 · 6 citationsarXiv
Synthetic observations of dust emission and polarisation of Galactic cold clumps1908.03421v1 · Mika Juvela, Paolo Padoan, Isabelle Ristorcelli et al.2019 · 8 citationsarXiv
The Probability Distribution of Density Fluctuations in Supersonic Turbulence1905.00923v1 · Liubin Pan, Paolo Padoan, \AAke Nordlund2019 · 36 citationsarXiv
The CARMA-NRO Orion Survey: The filamentary structure as seen in CO emission1901.00176v1 · S. T. Suri, A. Sanchez-Monge, P. Schilke et al.2019 · 72 citationsA&A 623, A142 (2019)
Expanding associations in the Vela-Puppis region: 3D structure and kinematics of the young population1812.08114v2 · T. Cantat-Gaudin, C. Jordi, N. J. Wright et al.2018 · 105 citationsA&A 626, A17 (2019)
Dust polarisation studies on MHD simulations of molecular clouds: methods comparison for the relative orientations analysis1810.10014v1 · Elisabetta R. Micelotta, Mika Juvela, Paolo Padoan et al.2018 · 7 citationsA&A 647, A121 (2021)
The CARMA-NRO Orion Survey1803.11522v1 · Shuo Kong, H'ector G. Arce, Jesse R. Feddersen et al.2018 · 86 citationsarXiv
The magnetic field of molecular clouds1712.03408v1 · Paolo Padoan2017 · 1 citationarXiv
The stellar IMF from Isothermal MHD Turbulence1709.01078v2 · Troels Haugb\olle, Paolo Padoan, Aake Nordlund2017 · 85 citationsarXiv
Protostellar accretion traced with chemistry: Comparing synthetic C18O maps of embedded protostars to real observations1512.00416v2 · S\oren Frimann, Jes K. J\orgensen, Paolo Padoan et al.2015 · 26 citationsA&A 587, A60 (2016)
Supernova Driving. I. The Origin of Molecular Cloud Turbulence1509.04663v2 · Paolo Padoan, Liubin Pan, Troels Haugboelle et al.2015 · 222 citationsarXiv
The relative and absolute ages of old globular clusters in the LCDM framework1502.02670v2 · Michele Trenti, Paolo Padoan, Raul Jimenez2015 · 79 citationsThe Astrophysical Journal Letters. 808, L35, 2015
Turbulence-Induced Relative Velocity of Dust particles IV: the Collision Kernel1410.1989v1 · Liubin Pan, Paolo Padoan2014 · 42 citationsarXiv
Infall-Driven Protostellar Accretion and the Solution to the Luminosity Problem1407.1445v3 · Paolo Padoan, Troels Haugb\olle, \AAke Nordlund2014 · 114 citationsarXiv
The Star Formation Rate of Molecular Clouds1312.5365v1 · Paolo Padoan, Christoph Federrath, Gilles Chabrier et al.2013 · 73 citationsarXiv
Zooming in on the Formation of Protoplanetary Disks1309.2278v2 · A. Nordlund (1, T. Haugboelle, M. Kuffmeier (1 et al.2013 · 11 citationsarXiv
Turbulence-Induced Relative Velocity of Dust Particles I: Identical Particles1305.0307v2 · Liubin Pan, Paolo Padoan2013 · 73 citationsarXiv
A Simple Law of Star Formation1208.3758v2 · Paolo Padoan, Troels Haugboelle, AAke Nordlund2012 · 188 citationsarXiv
The Two States of Star Forming Clouds1202.2594v1 · David Collins, Alexei G. Kritsuk, Paolo Padoan et al.2012 · 142 citationsarXiv
The observable prestellar phase of the IMF1108.2543v2 · Paolo Padoan, AAke Nordlund2011 · 48 citationsarXiv
Turbulent Clustering of Protoplanetary Dust and Planetesimal Formation1106.3695v1 · Liubin Pan, Paolo Padoan, John Scalo et al.2011 · 102 citationsarXiv
Comparing Numerical Methods for Isothermal Magnetized Supersonic Turbulence1103.5525v2 · Alexei G. Kritsuk, Aake Nordlund, David Collins et al.2011 · 133 citationsAstrophysical Journal, 737, 13 (2011)
Pop. III stars from turbulent fragmentation at redshift ~ 111101.5163v1 · Joaquin Prieto, Paolo Padoan, Raul Jimenez et al.2011 · 30 citationsApJL, 731, 38 (2011)
Accuracy of core mass estimates in simulated observations of dust emission1009.4580v2 · J. Malinen, M. Juvela, D. C. Collins et al.2010 · 88 citationsA&A, 530 (2011), A101
Mass and Magnetic distributions in Self Gravitating Super Alfvenic Turbulence with AMR1008.2402v3 · David C. Collins, Paolo Padoan, Michael L. Norman et al.2010 · 57 citationsarXiv
Relative Velocity of Inertial Particles in Turbulent Flows1005.2419v1 · Liubin Pan, Paolo Padoan2010 · 76 citationsarXiv
Self-organization in Turbulent Molecular Clouds: Compressional versus Solenoidal Modes0912.0546v1 · Alexei G. Kritsuk, Sergey D. Ustyugov, Michael L. Norman et al.2009 · 8 citationsASP Conf.Ser.429:15-21,2010
The Power Spectrum of Turbulence in NGC 1333: Outflows or Large-Scale Driving?0910.1384v2 · Paolo Padoan, Mika Juvela, Alexei G. Kritsuk et al.2009 · 97 citationsAstrophys.J.707:L153-L157,2009
The IMF of stellar clusters: effects of accretion and feedback0908.4522v3 · Sami Dib, Mohsen Shadmehri, Paolo Padoan et al.2009 · 57 citationsarXiv
Simulating Supersonic Turbulence in Magnetized Molecular Clouds0908.0378v1 · Alexei G. Kritsuk, Sergey D. Ustyugov, Michael L. Norman et al.2009 · 31 citationsJournal of Physics: Conf. Ser., 180, 012020 (2009)
The Super-Alfvénic Model of Molecular Clouds: Predictions for Mass-to-Flux and Turbulent-to-Magnetic Energy Ratios0907.0587v2 · Tuomas Lunttila, Paolo Padoan, Mika Juvela et al.2009 · 35 citationsAstrophys.J.702:L37-L41,2009
The Star Formation Rate of Supersonic MHD Turbulence0907.0248v4 · Paolo Padoan, AAke Nordlund2009 · 520 citationsAstrophys.J.730:40,2011
Bridging the Gap Between Stars and Planets: The Formation and Early Evolution of Brown Dwarfs0903.2511v2 · Subhanjoy Mohanty, Adam Burgasser, Gilles Chabrier et al.2009 · 0 citationsarXiv
Simulations of Supersonic Turbulence in Molecular Clouds: Evidence for a New Universality0902.3222v2 · Alexei G. Kritsuk, Sergey D. Ustyugov, Michael L. Norman et al.2009 · 5 citationsASP Conf. Series, 406, 15-22 (2009)
Dissipative structures in supersonic turbulence.19257357 · Pan, Liubin, Padoan, Paolo, Kritsuk, Alexei G2009 · 37 citationsPhysical review letters. 2009;102(3):034501
The Temperature of Interstellar Clouds from Turbulent Heating0806.4970v3 · Liubin Pan, Paolo Padoan2008 · 77 citationsAstrophys.J.692:594-607,2009
The Super-Alfvénic Model of Molecular Clouds: Predictions for Zeeman Splitting Measurements0806.3854v2 · Tuomas Lunttila, Paolo Padoan, Mika Juvela et al.2008 · 31 citationsAstrophysical Journal Letters 686 (2008) L91-L94
Career total: at least 175 works. 94 are in this corpus.Showing the 50 most recent.
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