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P. J. Smith

3 papers here

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

author position
  • middle author2
  • last author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
ORCID 0000-0002-7489-5244

identity via Semantic Scholar / OpenAlex

most citedMultimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M⊙​

23 citations · 35 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2025

oMEGACat. VII. Tracing Interstellar and Intracluster Medium of ω Centauri using Sodium Absorptions

Z. Wang, A. C. Seth, M. Latour +14

We investigate the foreground interstellar medium along the line of sight and intracluster medium of ω Centauri (ω Cen) by measuring the equivalent width of Na I D absorptions…

astro-ph.GA2025★ 12 cited

oMEGACat. VI. Analysis of the overall kinematics of Omega Centauri in 3D: velocity dispersion, kinematic distance, anisotropy, and energy equipartition

Maximilian Häberle, Nadine Neumayer, Callie Clontz +15

Omega Centauri (ω Cen) is the Milky Way's most massive globular cluster and is likely the stripped nucleus of an accreted dwarf galaxy. In this paper, we analyze ω Cen's kinema…

astro-ph.GA2023★ 23 cited

Multimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M⊙​

Nolan Dickson, Vincent Hénault-Brunet, Holger Baumgardt +2

The distribution of stars and stellar remnants (white dwarfs, neutron stars, black holes) within globular clusters holds clues about their formation and long-term evolution, with i…

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