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20242026
most citedNumerical Insights into Disk Accretion, Eccentricity, and Kinematics in the Class 0 phase

2 citations · 2 across the 1 of their papers we have counts for

collaborators

6 papers

astro-ph.SR20262 cited

Numerical Insights into Disk Accretion, Eccentricity, and Kinematics in the Class 0 phase

Adnan Ali Ahmad, Benoît Commerçon, Elliot Lynch +4

The formation and early evolution of protoplanetary disks are governed by a wide variety of physical processes during a gravitational collapse. Observations have begun probing disk…

astro-ph.SR2025

Turn up the light: Radiative efficiency of protostars at birth

Asmita Bhandare, Adnan Ali Ahmad, Benoît Commerçon

Early stages of stellar birth comprise of a two-step process involving the formation of two hydrostatic cores. The second step of gravitational collapse sets the radiative efficien…

astro-ph.SR2025

Brown Dwarf Formation Through Gravitational Collapse: Insights From 3D Numerical Simulations

Adnan Ali Ahmad, Benoît Commerçon, Gilles Chabrier +1

The formation mechanism of Brown Dwarfs (BDs), whether akin to stars or ejected planetary-mass objects, remains debated. We present the first 3D radiation-MHD simulations of magnet…

astro-ph.SR2025

Birth of magnetized low-mass protostars and circumstellar disks

Adnan Ali Ahmad, Matthias González, Patrick Hennebelle +2

Although protostars and disks are often studied separately owing to numerical and observational challenges, breakthroughs in recent years have highlighted the need to study both ob…

astro-ph.EP2024

Formation and evolution of a protoplanetary disk: combining observations, simulations and cosmochemical constraints

Alessandro Morbidelli, Yves Marrocchi, Adnan Ali Ahmad +12

We present a plausible and coherent view of the evolution of the protosolar disk that is consistent with the cosmochemical constraints and compatible with observations of other pro…

astro-ph.SR2024

Formation of low mass protostars and their circumstellar disks

Adnan Ali Ahmad, Matthias González, Patrick Hennebelle +1

The birth process of circumstellar disks remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, o…