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S. Zwart

69 papers hereh-index 5811.9k citations360 works total

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

author position
  • sole author4
  • first author16
  • middle author22
  • last author12

Across the 54 of 69 papers where every author was matched, so the position is known.

fields
  • astro-ph66
  • astro-ph.GA1
  • astro-ph.SR1
  • cond-mat.other1
same name
  • S. Zwart — 1 paper, h 7

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
19972009
most citedStar cluster disruption by giant molecular clouds

276 citations · 1.9k across the 36 of their papers we have counts for

collaborators
Showing 1998Show all

4 papers · 1 filter

astro-ph1998

Star cluster ecology III: Runaway collisions in young compact star clusters

Simon Portegies Zwart, Junichiro Makino, Stephen L. W. McMillan +1

The evolution of young compact star clusters is studied using N-body simulations in which both stellar evolution and physical collisions between stars are taken into account. The i…

astro-ph1998

On the dissolution of evolving star clusters

Simon Portegies Zwart, Piet Hut, Junichiro Makino +1

Using direct N-body simulations which include both the evolution of single stars and the tidal field of the parent galaxy, we study the dynamical evolution of globular clusters and…

astro-ph1998

Gamma-ray bursts and density evolution of neutron star binary mergers

Philippe Bagot, Simon F. Portegies Zwart, Lev R. Yungelson

The evolution of the comoving cosmic merger-rate density of neutron star binaries n_c(z) is calculated using a distribution of their merging times provided by population-synthesis…

astro-ph1998

Evolution of Close Binaries: Formation and Merger of Neutron Star Binaries

Lev Yungelson, Simon F. Portegies Zwart

We discuss the formation and evolution of binaries which contain neutron stars or black holes. It is shown that in a stellar system which for 1010 yr had star formation rate s…

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