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A. Milone

3 papers here

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

author position
  • middle author3

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

fields
  • astro-ph.GA3
same name
  • A. Milone — 99 papers, h 64
  • A. Milone — 3 papers, h 6
  • A. Milone — 2 papers, h 8
  • A. Milone — 2 papers
  • A. Milone — 2 papers, h 2
  • A. Milone — 1 paper

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

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

12 citations · 12 across the 2 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.GA2024

oMEGACat V: Helium Enrichment in ω Centauri as a Function of Metallicity

C. Clontz, A. C. Seth, Z. Wang +12

Constraining the helium enhancement in stars is critical for understanding the formation mechanisms of multiple populations in star clusters. However, measuring helium variations f…

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