activity
19952026
most citedThe Stellar IMF from Turbulent Fragmentation

1k citations · 9k across the 113 of their papers we have counts for

collaborators

114 papers

astro-ph.GA2026

Hub-filament systems and the growth of massive stars: episodic accretion, clustered environments, and projection effects

Dana Makarova, Dana Alina, Paolo Padoan +4

The processes controlling the early mass growth of future massive stars remain poorly understood, particularly the connection of this growth to star clustering and hub-filament sys…

astro-ph.GA2026★ 4 cited

Random gas motions inside sub-parsec scale supercritical filaments

Chao Zhang, Tie Liu, Mika Juvela +12

Supercritical gas filaments in molecular clouds host the dense cores in which new stars form. The mechanisms governing their formation and subsequent gas accretion remain poorly un…

astro-ph.SR2026

Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales

Paolo Padoan, Mark Gieles

We revisit the luminosity function (LF) of compact HII regions in the context of the inertial--inflow model (IIM), in which massive stars assemble over extended, mass-dependent tim…

astro-ph.GA2025★ 1 cited

Globular cluster formation from inertial inflows: accreting extremely massive stars as the origin of abundance anomalies

Mark Gieles, Paolo Padoan, Corinne Charbonnel +2

We use the inertial-inflow model of massive star formation to describe the formation of globular clusters (GCs) in turbulent molecular clouds. A key aspect of this model is that th…

astro-ph.GA2024★ 13 cited

The Formation of Protoplanetary Disks through Pre-Main Sequence Bondi-Hoyle Accretion

Paolo Padoan, Liubin Pan, Veli-Matti Pelkonen +2

Protoplanetary disks are traditionally described as finite mass reservoirs left over by the gravitational collapse of the protostellar core, a view that strongly constrains both di…

astro-ph.GA2024

Updated kinematics of the Radcliffe Wave: non-synchronous, dipole-like vertical oscillations

Zhi-Kai Zhu, Min Fang, Zu-Jia Lu +6

The kinematic information of the Radcliffe Wave (RW) is essential for determining its existence and gaining insights into its origin and evolution. In this work, we present an accu…