most citedA Bending in the Size-mass Relation of Star-forming Galaxies across at a Critical Stellar Mass of Revealed by JWST

1 citations · 2 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2026

Evidence for the transformation from lenticular to spiral galaxies

Mengkui Zhou, Huiyuan Wang, Ran Li +8

It is widely accepted that late-type galaxies, such as spirals, evolve into early-type systems, including elliptical and lenticular galaxies, through galaxy mergers and violent dis…

astro-ph.GA20261 cited

A Bending in the Size-mass Relation of Star-forming Galaxies across at a Critical Stellar Mass of Revealed by JWST

Longyue Chen, Tao Wang, Hanwen Sun +12

We investigate the rest-frame optical size-stellar mass relation of galaxies at using deep JWST/NIRCam and MIRI imaging from the PRIMER survey. We find that star-formin…

astro-ph.GA2026

Interpreting the strong clustering of ultra-diffuse galaxies by halo spin bias

Qinglin Ma, Cheng Li, Yangyao Chen +1

We use the IllustrisTNG300-ODM simulation to investigate the spin bias of low-mass halos and its connection to the strong clustering of ultra-diffuse galaxies (UDGs) reported by Zh…

astro-ph.GA20261 cited

A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos

Yangyao Chen, Houjun Mo, Huiyuan Wang

We present a theoretical framework for seeding and growing supermassive black holes (SMBHs) in dark matter halos along their assembly histories. Seeds are bred out of Pop-III stars…

astro-ph.GA20261 cited

Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos

Qinglin Ma, Yangyao Chen, Houjun Mo

We use FIRE-2 cosmological zoom-in hydrodynamic simulations to investigate the co-evolution between Milky Way-size galaxies and their host dark matter halos. We find that the forma…

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…