activity
20142026
most citedSurface Brightness Profile of the Milky Way's Nuclear Star Cluster

208 citations · 1.1k across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.GA2026

SDSS-V Local Volume Mapper (LVM): The Integrated Light and Internal Rotation of Omega Centauri

Maximilian Häberle, Dmitry Bizyaev, Alina Boecker +34

The SDSS-V Local Volume Mapper (LVM) is a wide-field integral field spectroscopic survey of the Southern Milky Way plane, the Magellanic Clouds, and nearby Local Group galaxies. We…

astro-ph.GA2025★ 7 cited

Dynamical mass distribution and velocity structure of the Galactic centre

A. Feldmeier-Krause, T. Veršič, G. van de Ven +2

The inner ~200 pc region of the Milky Way contains a nuclear stellar disc and a nuclear star cluster that are embedded in the larger Galactic bar. These stellar systems overlap spa…

astro-ph.GA2025★ 9 cited

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,…

astro-ph.IM2025★ 11 cited

WIggle Corrector Kit for NIRSpEc Data: WICKED

Antoine Dumont, Nadine Neumayer, Anil C. Seth +8

The point-spread function of the integral-field unit (IFU) mode of the JWST's NIRSpec is heavily under-sampled, creating resampling noise seen as low-frequency sinusoidal-like arti…

astro-ph.GA2021★ 6 cited

A Giant Molecular Cloud Catalog in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)

E. R. Miura, D. Espada, A. Hirota +17

We present the first census of giant molecular clouds (GMCs) complete down to 10 and within the inner 4 kpc of the nearest giant elliptical and powerful radio galaxy,…

astro-ph.GA2021★ 21 cited

Distance to three molecular clouds in the central molecular zone

Francisco Nogueras-Lara, Rainer Schödel, Nadine Neumayer +1

The determination of absolute and relative distances of molecular clouds along the line-of-sight towards the central molecular zone (CMZ) is crucial to infer its orbital structure,…