Results 21 to 30 of about 273,575 (267)
On the formation of dwarf galaxies and stellar haloes [PDF]
15 pages, 7 figures, one figure added to match accepted version. Some typos fixed.
Read J. I, Pontzen A. P, Viel, Matteo
openaire +6 more sources
Mass Dependence of Galaxy–Halo Alignment in LOWZ and CMASS
We measure the galaxy-ellipticity (GI) correlations for the Sloan Digital Sky Survey Data Release 12 LOWZ and CMASS samples with the shape measurements from the DESI Legacy Imaging Surveys.
Kun Xu, Y. P. Jing, Hongyu Gao
doaj +1 more source
The elusive stellar halo of the Triangulum galaxy [PDF]
17 pages, 23 figures, accepted for publication in ...
Mcmonigal, B. +9 more
openaire +5 more sources
The extended ‘stellar halo’ of the Ursa Minor dwarf galaxy
ABSTRACT Stellar candidates in the Ursa Minor (UMi) dwarf galaxy have been found using a new Bayesian algorithm applied to Gaia EDR3 data. Five of these targets are located in the extreme outskirts of UMi, from ∼5 to 12 elliptical half-light radii (rh), where rh(UMi) = 17.32 ± 0.11 arcmin, and have been observed with the high-resolution ...
Federico Sestito +11 more
openaire +5 more sources
Feedback and the formation of dwarf galaxy stellar haloes [PDF]
Stellar population studies show that low mass galaxies in all environments exhibit stellar halos that are older and more spherically distributed than the main body of the galaxy. In some cases, there is a significant intermediate age component that extends beyond the young disk. We examine a suite of Smoothed Particle Hydrodynamic (SPH) simulations and
Stinson, Greg +5 more
openaire +2 more sources
Halo Properties from Observable Measures of Environment: I. Halo and Subhalo Masses
The stellar mass - halo mass relation provides a strong basis for connecting galaxies to their host dark matter halos in both simulations and observations.
Haley Bowden +2 more
doaj +1 more source
Stellar haloes of disc galaxies at z ∼ 1 [PDF]
14 pages, 14 figures. Accepted in MNRAS.
Trujillo, I, Bakos, Judit
openaire +3 more sources
Decoding Galactic Merger Histories
Galaxy mergers are expected to influence galaxy properties, yet measurements of individual merger histories are lacking. Models predict that merger histories can be measured using stellar halos and that these halos can be quantified using observations of
Eric F. Bell +7 more
doaj +1 more source
A ‘Universal’ Density Profile for the Outer Stellar Halos of Galaxies [PDF]
AbstractThe outer stellar halos of galaxies contain vital information about the formation history of galaxies, since the relaxation timescales in the outskirts are long enough to keep the memory, while the information about individual formation events in the central parts has long been lost due to mixing, star formation and relaxation.
Remus, R., Burkert, A., Dolag, K.
openaire +4 more sources
Studying stellar halos with future facilities [PDF]
Stellar halos around galaxies retain fundamental evidence of the processes which lead to their build up. Sophisticated models of galaxy formation in a cosmological context yield quantitative predictions about various observable characteristics, including
GREGGIO, Laura +2 more
core +1 more source

