collaborators

5 papers

astro-ph.GA2026

Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5

Boris S. Kalita, Luis C. Ho, John D. Silverman +6

In this work, we explore the nature of galactic bars. Once thought to be highly transient, our results demonstrate otherwise. Our sample consists of nine massive ($>10^{10.5}…

astro-ph.GA2025

The role of environment on the evolution of disc galaxies density profiles New insights from simulations and comparison to Euclid data

M. Mondelin, F. Bournaud, J-C. Cuillandre +1

Galactic discs are known to have exponential radial profiles in luminosity and stellar surface density in their bright inner regions. Nonetheless, their faint outer regions often d…

astro-ph.GA2025

Euclid: Early Release Observations -- The surface brightness and colour profiles of the far outskirts of galaxies in the Perseus cluster

M. Mondelin, F. Bournaud, J. -C. Cuillandre +110

The Perseus field captured by Euclid as part of its Early Release Observations provides a unique opportunity to study cluster environment ranging from outskirts to dense regions. L…

astro-ph.GA2025

On the origin of compressive turbulence in protoclumps in high redshift disks

Omry Ginzburg, Avishai Dekel, Nir Mandelker +4

The giant, star forming clumps in gas-rich, high redshift disks are commonly assumed to form due to gravitational instabilities, in which protoclumps have a Toomre- parameter le…

astro-ph.GA2025

Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament

Maryam Arabsalmani, Sambit Roychowdhury, Benjamin Schneider +11

We identify a chain of galaxies along an almost straight line in the nearby Universe with a projected length of ~5 Mpc. The galaxies are distributed within projected distances of o…