activity
20242026
collaborators

5 papers

astro-ph.GA2026

Satellite quenching by radio jets of central galaxies in galaxy groups

Yijun Wang, Tao Wang, Dingyi Zhao +9

Feedback from active galactic nuclei (AGN) is now recognized as a key component of galaxy formation models. It plays a central role in regulating the growth and quenching of galaxi…

astro-ph.GA2026

Radio AGN feedback sustains quiescence only in a minority of massive galaxies

Huiling Liu, Yan Lu, Hui Hong +11

Radio active galactic nuclei (AGNs) eject a huge amount of energy into the surrounding medium and are thought to potentially prevent gas cooling and maintain the quiescence of mass…

astro-ph.CO2025

Unexpected clustering pattern in dwarf galaxies challenges formation models

Ziwen Zhang, Yangyao Chen, Yu Rong +4

The galaxy correlation function serves as a fundamental tool for studying cosmology, galaxy formation, and the nature of dark matter. It is well established that more massive, redd…

astro-ph.GA2025

Measuring Mass of Gas in Central Galaxies using weak lensing and satellite kinematics in MOND

Li Ma, Ziwen Zhang, Huiyuan Wang +1

In Milgrom's modified Newtonian dynamics (MOND) framework, the dynamical mass of a galaxy is fully determined by its baryonic matter distribution. We fit the distribution of cold a…

astro-ph.CO2024

UNIONS: a direct measurement of intrinsic alignment with BOSS/eBOSS spectroscopy

Fabian Hervas Peters, Martin Kilbinger, Romain Paviot +12

During their formation, galaxies are subject to tidal forces, which create correlations between their shapes and the large-scale structure of the Universe, known as intrinsic align…