Baryonic solutions and challenges for cosmological models of dwarf galaxies

LV Sales, A Wetzel, A Fattahi - Nature Astronomy, 2022 - nature.com
Galaxies and their dark-matter haloes have posed several challenges to the dark energy
plus cold dark matter (Λ CDM) cosmological model. These discrepancies between …

Illuminating low surface brightness galaxies with the Hyper Suprime-Cam survey

JP Greco, JE Greene, MA Strauss… - The Astrophysical …, 2018 - iopscience.iop.org
We present a catalog of extended low surface brightness galaxies (LSBGs) identified in the
Wide layer of the Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP). Using the …

The origin of ultra diffuse galaxies: stellar feedback and quenching

TK Chan, D Kereš, A Wetzel, PF Hopkins… - Monthly Notices of …, 2018 - academic.oup.com
We test if the cosmological zoom-in simulations of isolated galaxies from the FIRE project
reproduce the properties of ultra diffuse galaxies (UDGs). We show that outflows that …

The Next Generation Virgo Cluster Survey (NGVS). XXX. Ultra-diffuse galaxies and their globular cluster systems

S Lim, P Côté, EW Peng, L Ferrarese… - The Astrophysical …, 2020 - iopscience.iop.org
The Next Generation Virgo Cluster Survey (NGVS). XXX. Ultra-diffuse Galaxies and Their
Globular Cluster Systems - IOPscience This site uses cookies. By continuing to use this site you …

Systematically Measuring Ultra-diffuse Galaxies (SMUDGes). V. The Complete SMUDGes Catalog and the Nature of Ultradiffuse Galaxies

D Zaritsky, R Donnerstein, A Dey… - The Astrophysical …, 2023 - iopscience.iop.org
We present the completed catalog of ultradiffuse galaxy (UDG) candidates (7070 objects)
from our search of the DR9 Legacy Survey images, including distance and total mass …

[HTML][HTML] The Fornax Deep Survey with VST-III. Low surface brightness dwarfs and ultra diffuse galaxies in the center of the Fornax cluster

A Venhola, R Peletier, E Laurikainen, H Salo… - Astronomy & …, 2017 - aanda.org
Context. Studies of low surface brightness (LSB) galaxies in nearby clusters have revealed a
sub-population of extremely diffuse galaxies with central surface brightness of μ 0, g′> 24 …

The formation of ultradiffuse galaxies in clusters

LV Sales, JF Navarro, L Penafiel… - Monthly Notices of …, 2020 - academic.oup.com
We use the IllustrisTNG cosmological hydrodynamical simulation to study the formation of
ultradiffuse galaxies (UDGs) in galaxy clusters. We supplement the simulations with a …

The formation of ultra-diffuse galaxies in cored dark matter haloes through tidal stripping and heating

T Carleton, R Errani, M Cooper… - Monthly Notices of …, 2019 - academic.oup.com
We propose that the ultra-diffuse galaxy (UDG) population represents a set of satellite
galaxies born in∼ 1010− 1011 M⊙ haloes, similar to field dwarfs, which suffer a dramatic …

Spatially resolved stellar kinematics of the ultra-diffuse galaxy dragonfly 44. I. Observations, kinematics, and cold dark matter halo fits

P Van Dokkum, A Wasserman, S Danieli… - The Astrophysical …, 2019 - iopscience.iop.org
We present spatially resolved stellar kinematics of the well-studied ultra-diffuse galaxy
(UDG) Dragonfly 44, as determined from 25.3 hr of observations with the Keck Cosmic Web …

Origin and evolution of ultradiffuse galaxies in different environments

JA Benavides, LV Sales, MG Abadi… - Monthly Notices of …, 2023 - academic.oup.com
We study the formation of ultradiffuse galaxies (UDGs) using the cosmological
hydrodynamical simulation TNG50 of the Illustris-TNG suite. We define UDGs as dwarf …