Shantanu Basu

Professor

University of Western Ontario Faculty of Science

Canada

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About

Shantanu Basu is a Professor at the University of Western Ontario Faculty of Science, Canada. His research focuses on protoplanetary disks, star formation, and the effects of magnetic fields in astrophysical environments. Recent contributions include development of simulation codes for understanding protoplanetary disk evolution and investigating accretion phenomena in young stars.

Articles (20)

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2025

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2021

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2021

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2021

Collaborators (4)

Christoph Federrath

Australian National University

AUSTRALIA

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Daniele Galli

Contract Professor Course Physics of Interstellar Medium

University of Florence

ITALY

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Josep Miquel Girart

Investigador Científico / Professor

Institut de Ciències del Mar

SPAIN

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Shingo Hirano

Assistant Professor

Kanagawa University

JAPAN

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Shantanu Basu

Research Interests

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About

Articles (20)

Development of 1D Non-ideal MHD Simulation Code Towards understanding Long-term Evolution of Protoplanetary Disk

Effect of Magnetic Field on the Accretion Phase of Population III Star Formation

Accretion Bursts in Young Intermediate-mass Stars Make Planet Formation Challenging

Projection-angle effects when “observing” a turbulent magnetized collapsing molecular cloud

Magnetic disk winds in protoplanetary disks

Projection-angle effects when “observing” a turbulent magnetized collapsing molecular cloud

Complex Structure around a Circumstellar Disk Caused by Interchange Instability

Magnetic Fields in Massive Star-forming Regions (MagMaR): Unveiling an Hourglass Magnetic Field in G333.46–0.16 Using ALMA

Cloud Dissipation and Disk Wind in the Late Phase of Star Formation

GRINN: a physics-informed neural network for solving hydrodynamic systems in the presence of self-gravity

Magnetic Effects Promote Supermassive Star Formation in Metal-enriched Atomic-cooling Halos

Can we observe the ion-neutral drift velocity in prestellar cores?

Primordial dusty rings and episodic outbursts in protoplanetary discs

Synthetic Polarization Maps of an Outflow Zone from Magnetohydrodynamic Simulations

A semi-analytical model for the temporal evolution of the episodic disc-to-star accretion rate during star formation

The Magnetic Field versus Density Relation in Star-forming Molecular Clouds

Magnetic Properties of Star-forming Dense Cores

Supermassive Star Formation in Magnetized Atomic-cooling Gas Clouds: Enhanced Accretion, Intermittent Fragmentation, and Continuous Mergers

Effect of mass-loss due to stellar winds on the formation of supermassive black hole seeds in dense nuclear star clusters

Variation of the core lifetime and fragmentation scale in molecular clouds as an indication of ambipolar diffusion

Collaborators (4)

Christoph Federrath

Daniele Galli

Josep Miquel Girart

Shingo Hirano

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