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researcher

J. Hurley

5 papers hereh-index 363 citations5 works total

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

author position
  • middle author4
  • last author1

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph1
  • astro-ph.HE1
same name
  • J. Hurley — 78 papers, h 38
  • J. Hurley — 4 papers, h 4
  • J. Hurley — 2 papers, h 18
  • J. Hurley — 1 paper, h 18
  • J. Hurley — 1 paper, h 4

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
20082026
most citedEvolution of stellar collision products in open clusters. I. Blue stragglers in N-body models of M67

67 citations · 95 across the 5 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.HE2025

Modelling Millisecond Pulsar Populations in Globular Clusters with NBODY6++GPU

Yuzhe Song, Debatri Chattopadhyay, Jarrod Hurley +3

Millisecond pulsars (MSPs) are neutron stars with spin periods as short as a few milliseconds, formed through mass accretion from companion stars. In the dense environments of glob…

astro-ph.GA2025★ 12 cited

Efficient black hole seed formation in low metallicity and dense stellar clusters with implications for JWST sources

M. C. Vergara, A. Askar, F. Flammini Dotti +7

Recent observations with the James Webb Space Telescope (JWST) reveal young massive clusters (YMCs) as key building blocks of early galaxies. They are not only important constituen…

astro-ph.GA2025★ 16 cited

Rapid formation of a very massive star >50000 M⊙​ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters

Marcelo C. Vergara, Abbas Askar, Albrecht W. H. Kamlah +15

Context. We present simulations of a massive young star cluster using \textsc{Nbody6++GPU} and \textsc{MOCCA}. The cluster is initially more compact than previously published model…

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