activity
20242026
collaborators

6 papers

astro-ph.GA2026

Little Red Dot progenitors from Compact Starbursts: A Natural Path to Early AGN Formation

Matías Liempi, Muhammad A. Latif, Dominik R. G. Schleicher

The recent discovery of Little Red Dots (LRDs) by the James Webb Space Telescope has challenged traditional models of early galaxy and black hole co-evolution. The nature of these…

astro-ph.GA2026

Formation of intermediate-mass black holes in young massive clusters detected with JWST: analytic mass estimates

Viola Bocchi, Matías Liempi, Dominik R. G. Schleicher

The James Webb Space Telescope (JWST) has revealed a population of dense stellar systems at high redshift, including the "Cosmic Gems" arc () and the "Firefly Sparkle"…

astro-ph.GA2026

Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes

Dominik R. G. Schleicher, Matías Liempi, Mirek Giersz +11

The James Webb Space Telescope (JWST) has detected, through gravitational lensing, several young massive star clusters (YMCs), which are considered as relevant building blocks of h…

astro-ph.GA2026

Constraints on dynamically-formed massive black holes in Little Red Dots from X-ray non-detections

M. Liempi, D. R. G. Schleicher, M. A. Latif +4

The existence of massive, compact galaxies (Little Red Dots, LRDs) at challenges early structure formation models, suggesting rapid stellar and black hole (BH) assembly.…

astro-ph.GA2025

On the Fate of Little Red Dots

Andres Escala, Lucas Zimmermann, Sebastian Valdebenito +3

We study the stability and possible fates of Little Red Dots, under the stellar-only interpretation of their observational features. This is performed by a combination of analyzing…

astro-ph.GA2024

The supermassive black hole population from seeding via collisions in Nuclear Star Clusters

M. Liempi, D. R. G. Schleicher, A. Benson +2

The coexistence of nuclear star clusters (NSCs) and supermassive black holes (SMBHs) in galaxies with stellar masses M, the scaling relations between their p…