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researcher

S. Chatterjee

4 papers hereh-index 448.2k citations174 works total

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

author position
  • first author3
  • middle author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.SR1
same name
  • S. Chatterjee — 16 papers, h 43
  • S. Chatterjee — 14 papers, h 53
  • S. Chatterjee — 4 papers, h 43
  • S. Chatterjee — 4 papers, h 7
  • S. Chatterjee — 4 papers, h 13
  • S. Chatterjee — 3 papers, h 15

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
20072009
most citedDynamical Outcomes of Planet-Planet Scattering

932 citations · 954 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2009★ 4 cited

On the Dynamical Evolution of the Arches Cluster

Sourav Chatterjee, Sanghamitra Goswami, Stefan Umbreit +3

We study the dynamical evolution of the young star cluster Arches and its dependence on the assumed initial stellar mass function (IMF). We perform many direct N-body simulations…

astro-ph2008★ 16 cited

Clearing the Dust from Globular Clusters

Stefan Umbreit, Sourav Chatterjee, Frederic A. Rasio

Recent Spitzer observations of the globular cluster M15 detected dust associated with its intracluster medium. Surprisingly, these observations imply that the dust must be very sho…

astro-ph2007★ 2 cited

Effects of stellar collisions on star cluster evolution and core collapse

Sourav Chatterjee, John M. Fregeau, Frederic A. Rasio

We systematically study the effects of collisions on the overall dynamical evolution of dense star clusters using Monte Carlo simulations over many relaxation times. We derive many…

astro-ph2007★ 932 cited

Dynamical Outcomes of Planet-Planet Scattering

Sourav Chatterjee, Eric B. Ford, Soko Matsumura +1

Observations in the past decade have revealed extrasolar planets with a wide range of orbital semimajor axes and eccentricities. Based on the present understanding of planet format…

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