collaborators

6 papers

astro-ph.GA2026

3D CMZ V: A new orbital model of our Galaxy's Center, informed by data across the electromagnetic spectrum

Dani R. Lipman, Cara Battersby, Daniel Walker +9

The 3D structure of The Milky Way's Central Molecular Zone (CMZ) informs our understanding of star formation cycles, black hole accretion, and the evolution of galactic nuclei. How…

astro-ph.HE2026

High Energy Emission from the Galactic Center

Andrea Goldwurm, Maïca Clavel, Stefano Gabici +1

The center of the Galaxy is a prominent source in X-rays and gamma-rays. The study of its high-energy (HE) emission is crucial in understanding the physical phenomena taking place…

astro-ph.HE2026

Direct detection of the non-thermal X-ray emission from the Arches star cluster

Roman Krivonos, Alexey Vikhlinin, Andrei Bykov +2

The compact stellar clusters have emerged as particularly promising candidates for cosmic rays (CR) accelerators. The star clusters, recently observed in gamma-rays, are also known…

astro-ph.GA2025

3D MC II: X ray echoes reveal a clumpy molecular cloud in the CMZ

Danya Alboslani, Cara Battersby, Samantha Brunker +3

X-ray observations collected over the last decades have revealed a strongly variable X-ray signal within the Milky Way's Galactic center, interpreted as X-ray echoes from its super…

astro-ph.GA2025

VLTI/GRAVITY upper limit on near-infrared emission from the nearby 33 Msun black hole Gaia BH3

Pierre Kervella, Pasquale Panuzzo, Alexandre Gallenne +11

The recent astrometric discovery of the nearby (590 pc) massive () dormant black hole candidate Gaia BH3 offers the possibility to angularly resolve the black hole from…

astro-ph.GA2025

3D MC I: X-ray Tomography Begins to Unravel the 3-D Structure of a Molecular Cloud in our Galaxy's Center

Samantha W. Brunker, Cara Battersby, Danya Alboslani +5

Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center. Mo…