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20242026
most citedoMEGACat. X. Shedding light on the disrupted dwarf galaxy of Omega Centauri

3 citations · 5 across the 4 of their papers we have counts for

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astro-ph.GA2025

Age, Chemistry, and Kinematics of the Inner Galaxy Revealed by MUSE

Zixian Wang, Michael R. Hayden, Sanjib Sharma +3

The bar/bulge and inner disk are fundamental building blocks of the Milky Way, containing a large fraction of its stellar mass. However, stars in these regions are faint, crowded,…

astro-ph.GA20251 cited

oMEGACat. VIII. A Subpopulation Census of ω Centauri

C. Clontz, A. C. Seth, Z. Wang +8

An understanding of the assembly history of the complex star cluster Omega Centauri has long been sought after, with many studies separating the stars on the color-magnitude diagra…

astro-ph.GA2025

oMEGACat. VII. Tracing Interstellar and Intracluster Medium of 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 Centauri ( Cen) by measuring the equivalent width of Na I D absorption…

astro-ph.GA2025

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 ( 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 Cen's kine…

astro-ph.GA2025

Studying Binary Systems in Omega Centauri with MUSE: II. Observational constraints on the orbital period distribution

S. Saracino, S. Kamann, F. Wragg +8

Omega Centauri ( Cen) is one of the most complex star clusters in the Milky Way, and likely the stripped nucleus of an accreted dwarf galaxy. Being the subject of debate betwee…

astro-ph.GA2025

A spectroscopic map of the Galactic centre -- Observations and resolved stars

A. Feldmeier-Krause, N. Neumayer, A. Seth +10

The Galactic Centre region contains a dense accumulation of stars, which can be separated into two components: A flattened and dense nuclear star cluster (NSC), and a surrounding,…