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researcher

S. Basu

59 papers hereh-index 363.9k citations176 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author3
  • first author8
  • middle author18
  • last author26

Across the 55 of 59 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR23
  • astro-ph17
  • astro-ph.GA15
  • astro-ph.EP3
  • physics.gen-ph1
same name
  • S. Basu — 111 papers, h 84
  • S. Basu — 39 papers, h 70
  • S. Basu — 27 papers, h 7
  • S. Basu — 18 papers
  • S. Basu — 17 papers, h 16
  • S. Basu — 17 papers, h 25

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19982026
most citedThe Burst Mode of Protostellar Accretion

381 citations · 1.2k across the 35 of their papers we have counts for

collaborators
Showing 2024Show all

4 papers · 1 filter

astro-ph.GA2024

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

Piyali Saha, Patricio Sanhueza, Marco Padovani +33

The contribution of the magnetic field to the formation of high-mass stars is poorly understood. We report the high-angular resolution (∼0.3′′, 870 au) map of the…

astro-ph.SR2024★ 3 cited

Hourglass Magnetic Field of a Protostellar System

Shantanu Basu, Xiyuan Li, Gianfranco Bino

An hourglass-shaped magnetic field pattern arises naturally from the gravitational collapse of a star-forming gas cloud. Most studies have focused on the prestellar collapse phase,…

astro-ph.SR2024

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

Masahiro N. Machida, Shantanu Basu

We perform a long-term simulation of star and disk formation using three-dimensional non-ideal magnetohydrodynamics. The simulation starts from a prestellar cloud and proceeds thro…

astro-ph.SR2024

Outflows Driven from a Magnetic Pseudodisk

Shantanu Basu, Mahmoud Sharkawi, Masahiro N. Machida

Outflows play a pivotal role in star formation as one of its most visible markers and a means of transporting mass, momentum, and angular momentum from the infalling gas into the s…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.