High-resolution mass models of dwarf galaxies from LITTLE THINGS
SH Oh, DA Hunter, E Brinks… - The Astronomical …, 2015 - iopscience.iop.org
We present high-resolution rotation curves and mass models of 26 dwarf galaxies from"
Local Irregulars That Trace Luminosity Extremes, The H i Nearby Galaxy Survey"(LITTLE …
Local Irregulars That Trace Luminosity Extremes, The H i Nearby Galaxy Survey"(LITTLE …
SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation
S McAlpine, JC Helly, M Schaller… - Monthly Notices of …, 2022 - academic.oup.com
We present sibelius-dark, a constrained realization simulation of the local volume to a
distance of 200 Mpc from the Milky Way. sibelius-dark is the first study of the 'Simulations …
distance of 200 Mpc from the Milky Way. sibelius-dark is the first study of the 'Simulations …
Density profile of dark matter haloes and galaxies in the horizon–agn simulation: the impact of AGN feedback
S Peirani, Y Dubois, M Volonteri… - Monthly Notices of …, 2017 - academic.oup.com
Using a suite of three large cosmological hydrodynamical simulations, horizon–agn, horizon–
noagn (no AGN feedback) and horizon–dm (no baryons), we investigate how a typical sub …
noagn (no AGN feedback) and horizon–dm (no baryons), we investigate how a typical sub …
Wide-field precision kinematics of the M87 globular cluster system
J Strader, AJ Romanowsky, JP Brodie… - The Astrophysical …, 2011 - iopscience.iop.org
We present the most extensive combined photometric and spectroscopic study to date of the
enormous globular cluster (GC) system around M87, the central giant elliptical galaxy in the …
enormous globular cluster (GC) system around M87, the central giant elliptical galaxy in the …
[HTML][HTML] Observational constraints on Yukawa cosmology and connection with black hole shadows
We confront Yukawa modified cosmology, proposed in Jusufi et al.[arXiv: 2304.11492], with
data from Supernovae Type Ia (SNe Ia) and Hubble parameter (OHD) observations. Yukawa …
data from Supernovae Type Ia (SNe Ia) and Hubble parameter (OHD) observations. Yukawa …
The effects of baryon physics, black holes and active galactic nucleus feedback on the mass distribution in clusters of galaxies
The spatial distribution of matter in clusters of galaxies is mainly determined by the dominant
dark matter component; however, physical processes involving baryonic matter are able to …
dark matter component; however, physical processes involving baryonic matter are able to …
Cusp–core transformations induced by AGN feedback in the progenitors of cluster galaxies
In a recent study, we used cosmological simulations to show that active galactic nuclei
(AGN) feedback on the gas distribution in clusters of galaxies can be important in …
(AGN) feedback on the gas distribution in clusters of galaxies can be important in …
Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster-I. Project description and preliminary results
E Iodice, M Hilker, G Doll, M Mirabile, C Buttitta… - Astronomy & …, 2023 - aanda.org
Looking into the faintEst WIth MUSE (LEWIS) is an ESO large observing programme that
aims at obtaining the first homogeneous integral-field spectroscopic survey of 30 extremely …
aims at obtaining the first homogeneous integral-field spectroscopic survey of 30 extremely …
Testing Yukawa cosmology at the Milky Way and M31 galactic scales
We address the galaxy rotation curves through the Yukawa gravitational potential emerging
as a correction of the Newtonian potential in extended theories of gravity. On the one hand …
as a correction of the Newtonian potential in extended theories of gravity. On the one hand …
[HTML][HTML] Dark Universe phenomenology from Yukawa potential?
We argue that the effect of cold dark matter in the cosmological setup can be explained by
the coupling between the baryonic matter particles in terms of the long-range force having a …
the coupling between the baryonic matter particles in terms of the long-range force having a …