activity
20242026
collaborators

5 papers

astro-ph.SR2026

MESA Isochrones and Stellar Tracks. II. Models with alpha-enhanced chemical composition

A Dotter, E Bauer, MJ Park +4

We update and expand the MESA Isochrones and Stellar Tracks (MIST) database to include variations in the alpha-capture elements, specifically [alpha/Fe]=-0.2, 0, +0.2, +0.4, and +0…

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

Fast-moving stars around an intermediate-mass black hole in Omega Centauri

Maximilian Häberle, Nadine Neumayer, Anil Seth +15

Black holes have been found over a wide range of masses, from stellar remnants with masses of 5-150 solar masses (Msun), to those found at the centers of galaxies with Msu…

astro-ph.GA2024

oMEGACat V: Helium Enrichment in 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…