Origins of the Evil Eye: M64's Stellar Halo Reveals the Recent Accretion of an SMC-mass Satellite
M64, often called the “Evil Eye” galaxy, is unique among local galaxies. Beyond its dramatic, dusty nucleus, it also hosts an outer gas disk that counter-rotates relative to its stars.
Adam Smercina +11 more
doaj +1 more source
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
Falomo, Renato +2 more
core +3 more sources
The Impact of Assembly Bias on the Galaxy Content of Dark Matter Halos [PDF]
We study the dependence of the galaxy content of dark matter halos on large-scale environment and halo formation time using semi-analytic galaxy models applied to the Millennium simulation.
I. Zehavi +5 more
semanticscholar +1 more source
The Colors of Dwarf Elliptical Galaxy Globular Cluster Systems, Nuclei, and Stellar Halos [PDF]
We present the results of a Hubble Space Telescope WFPC2 F555W and F814W survey of 69 dwarf elliptical galaxies (dEs) in the Virgo and Fornax Clusters and Leo Group.
J. Lotz, B. Miller, H. Ferguson
semanticscholar +1 more source
Tracing Galaxy Formation with Stellar Halos. II. Relating Substructure in Phase and Abundance Space to Accretion Histories [PDF]
This paper explores the mapping between the observable properties of a stellar halo in phase and abundance space and the parent galaxy’s accretion history in terms of the characteristic epoch of accretion and mass and orbits of progenitor objects.
K. Johnston +5 more
semanticscholar +1 more source
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
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 +4 more sources
Revealing the Galaxy–Halo Connection through Machine Learning
Understanding the connections between galaxy stellar mass, star formation rate, and dark matter halo mass represents a key goal of the theory of galaxy formation. Cosmological simulations that include hydrodynamics, physical treatments of star formation,
Ryan Hausen +7 more
doaj +1 more source
THE STELLAR HALOS OF MASSIVE ELLIPTICAL GALAXIES. III. KINEMATICS AT LARGE RADIUS [PDF]
We present a two-dimensional kinematic analysis out to ∼2–5 effective radii (Re) of 33 massive elliptical galaxies with stellar velocity dispersions σ > 150 km s−1.
S. Raskutti, J. Greene, J. Murphy
semanticscholar +1 more source
The Outer Halos of Very Massive Galaxies: BCGs and their DSC in the Magneticum Simulations
Recent hydrodynamic cosmological simulations cover volumes up to Gpc 3 and resolve halos across a wide range of masses and environments, from massive galaxy clusters down to normal galaxies, while following a large variety of physical processes ...
Rhea-Silvia Remus +2 more
doaj +1 more source

