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researcher

R. Banerjee

93 papers hereh-index 395.5k citations137 works total

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

author position
  • sole author1
  • first author12
  • middle author50
  • last author29

Across the 92 of 93 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA27
  • astro-ph.SR24
  • astro-ph17
  • astro-ph.CO16
  • astro-ph.IM3
  • astro-ph.EP2
same name
  • R. Banerjee — 155 papers, h 39
  • R. Banerjee — 18 papers, h 7
  • R. Banerjee — 15 papers, h 7
  • R. Banerjee — 11 papers, h 4
  • R. Banerjee — 11 papers, h 6
  • R. Banerjee — 9 papers, h 8

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
20002026
most citedModeling Collapse and Accretion in Turbulent Gas Clouds: Implementation and Comparison of Sink Particles in AMR and SPH

414 citations · 6.2k across the 93 of their papers we have counts for

collaborators
Showing 2016 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2016★ 96 cited

Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks

Mikhail Klassen, Ralph Pudritz, Rolf Kuiper +2

We present radiation hydrodynamic simulations of collapsing protostellar cores with initial masses of 30, 100, and 200 M⊙​. We follow their gravitational collapse and the f…

astro-ph.GA2016★ 51 cited

Supernova Feedback in Molecular Clouds: Global Evolution and Dynamics

Bastian Körtgen, Daniel Seifried, Robi Banerjee +2

We use magnetohydrodynamical simulations of converging warm neutral medium flows to analyse the formation and global evolution of magnetised and turbulent molecular clouds subject…

astro-ph.GA2016★ 17 cited

The formation of the primitive star SDSS J102915+172927: effect of the dust mass and the grain-size distribution

S. Bovino, T. Grassi, D. R. G. Schleicher +1

Understanding the formation of the extremely metal poor star SDSS-J102915+172927 is of fundamental importance to improve our knowledge on the transition between the first and secon…

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