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astro-ph.GA2024

A binary system in the S cluster close to the supermassive black hole Sagittarius A*

Florian Peißker, Michal Zajacek, Lucas Labadie +4

High-velocity stars and peculiar G objects orbit the central supermassive black hole (SMBH) Sagittarius A* (Sgr A*). Together, the G objects and high-velocity stars constitute the…

astro-ph.GA2024

MIRI Deep Imaging Survey (MIDIS) of the Hubble Ultra Deep Field

Göran Östlin, Pablo G. Pérez-González, Jens Melinder +41

The recently launched James Webb Space Telescope (JWST) is opening new observing windows on the distant universe. Among JWST's instruments, the Mid Infrared Instrument (MIRI) offer…

astro-ph.GA2024

JWST/MIRI unveils the stellar component of the GN20 dusty galaxy overdensity at =4.05

A. Crespo Gómez, L. Colina, J. Álvarez-Márquez +24

Despite the importance of the dusty star-forming galaxies (DSFGs) at >2 for understanding the galaxy evolution in the early Universe, their stellar distributions traced by the n…

astro-ph.GA2024

Discovery of a Dense Association of Stars in the Vicinity of the Supermassive Black Hole Sgr A*

S. Elaheh Hosseini, Andreas Eckart, Michal Zajaček +3

We focus on a sample of 42 sources in the vicinity of the bow-shock source IRS 1W (N-sources), located at the distance of north-east of the supermassive black hole (SMBH)…

astro-ph.GA2024

Dynamics of star associations in an SMBH-IMBH system: The case of IRS13 in the Galactic centre

Václav Pavlík, Vladimír Karas, Bhavana Bhat +2

Context: The existence of intermediate-mass black holes (IMBHs) still poses challenges to theoretical and observational astronomers. Several candidates have been proposed, includin…

astro-ph.GA2024

The Evaporating Massive Embedded Stellar Cluster IRS 13 Close to Sgr A*. II. Kinematic structure

Florian Peißker, Michal Zajacek, Matus Labaj +8

The existence of two distinct and apparently unrelated populations of dusty stellar objects in the Nuclear Stellar Cluster (NSC) of the Milky Way, namely IRS 13 and the S-cluster,…