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researcher

S. McMillan

12 papers hereh-index 61.1k citations17 works total

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

author position
  • middle author6
  • last author4

Across the 10 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA8
  • astro-ph1
  • astro-ph.CO1
  • astro-ph.IM1
  • gr-qc1
same name
  • S. McMillan — 63 papers, h 38
  • S. McMillan — 11 papers, h 11
  • S. McMillan — 2 papers, h 21
  • S. McMillan — 1 paper, h 1
  • S. McMillan — 1 paper, h 2

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
19942025
most citedYoung massive star clusters

1.2k citations · 1.6k across the 11 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.GA2024

Massive Star Cluster Formation with Binaries. I. Evolution of Binary Populations

Claude Cournoyer-Cloutier, Alison Sills, William E. Harris +7

We study the evolution of populations of binary stars within massive cluster-forming regions. We simulate the formation of young massive star clusters within giant molecular clouds…

astro-ph.GA2024★ 4 cited

Massive star cluster formation III. Early mass segregation during cluster assembly

Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +6

Mass segregation is seen in many star clusters, but whether massive stars form in the center of a cluster or migrate there dynamically is still debated. N-body simulations have sho…

astro-ph.GA2024★ 19 cited

Massive star cluster formation II. Runaway stars as fossils of sub-cluster mergers

Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +6

Two main mechanisms have classically been proposed for the formation of runaway stars. In the binary supernova scenario (BSS), a massive star in a binary explodes as a supernova, e…

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