collaborators

7 papers

astro-ph.GA2026

The Fornax Cluster VLT Spectroscopic Survey - V. Mass modelling of the BCG NGC 1399 out to 150 kpc

Avinash Chaturvedi, Nicola R. Napolitano, Michael Hilker +8

NGC 1399, the bright central galaxy of the Fornax cluster, hosts an extensive population of globular clusters (GCs) extending beyond 200 kpc into its outer halo, about 6.5 effectiv…

astro-ph.GA2026

Supermassive black holes in six triaxial galaxies: Insights from SINFONI and MUSE observations

Sabine Thater, Avinash Chaturvedi, Davor Krajnovic +5

Dynamical modelling can be used to constrain the masses of central black holes; however, modelling massive galaxies is challenging due to their complexity. In this work, we report…

astro-ph.GA2026

The complex history of NGC 1427A revealed by its star clusters and star formation history

Katja Fahrion, Michael Hilker, Avinash Chaturvedi +2

Star-forming low-mass galaxies in the dense environments of galaxy clusters provide opportunities to study how environmental effects such as ram-pressure stripping, tidal interacti…

astro-ph.GA2025

The Spatial Distribution of Intra-Cluster Globular Clusters in the Fornax Cluster

Raffaele D'Abrusco, Marco Mirabile, Michele Cantiello +6

We investigate the spatial distribution of the Intra-Cluster Globular Clusters (ICGCs) detected in the core of the Fornax galaxy cluster. By separately modeling different component…

astro-ph.CO2025

The SRG/eROSITA all-sky survey: View of the Fornax galaxy cluster

T. H. Reiprich, A. Veronica, F. Pacaud +18

The Fornax cluster is one of the closest X-ray-bright galaxy clusters. Previous observations of the intracluster medium were limited to less than R500. We aim to significantly exte…

astro-ph.HE2025

Searching for supermassive black holes binaries within SRG/eROSITA-De I: Properties of the X-ray selected candidates

D. Tubín-Arenas, M. Krumpe, D. Homan +20

Abridged: Supermassive black hole binaries (SMBHBs) separated by (sub)-pc scales represent one of the latest stages of hierarchical galaxy assembly. However, many of these objects…