Results 41 to 50 of about 173,239 (326)
Overview and public data release of the augmented Auriga Project: cosmological simulations of dwarf and Milky Way-mass galaxies [PDF]
We present an extended suite of the Auriga cosmological gravo-magnetohydrodynamical “zoom-in” simulations of 40 Milky Way-mass halos and 26 dwarf galaxy-mass halos run with the moving-mesh code arepo.
R. Grand +6 more
semanticscholar +1 more source
A time-resolved picture of our Milky Way’s early formation history [PDF]
The formation of our Milky Way can be split up qualitatively into different phases that resulted in its structurally different stellar populations: the halo and the disk components1–3.
M. Xiang, H. Rix
semanticscholar +1 more source
Evidence for two early accretion events that built the Milky Way stellar halo [PDF]
The Gaia Sausage is the major accretion event that built the stellar halo of the Milky Way galaxy. Here, we provide dynamical and chemical evidence for a second substantial accretion episode, distinct from the Gaia Sausage. The Sequoia Event provided the
G. Myeong +7 more
semanticscholar +1 more source
We describe an experiment to measure the mass of the Milky Way galaxy. The experiment is based on calculated light travel times along orthogonal directions in the Schwarzschild metric of the Galactic center. We show that the difference is proportional to
Angelo Tartaglia +14 more
core +1 more source
Kraken reveals itself – the merger history of the Milky Way reconstructed with the E-MOSAICS simulations [PDF]
Globular clusters (GCs) formed when the Milky Way experienced a phase of rapid assembly. We use the wealth of information contained in the Galactic GC population to quantify the properties of the satellite galaxies from which the Milky Way assembled ...
J. Kruijssen +8 more
semanticscholar +1 more source
The observed spiral structure of the Milky Way [PDF]
The spiral structure of the Milky Way is not yet well determined. The keys to understanding this structure are to increase the number of reliable spiral tracers and to determine their distances as accurately as possible.
Han, J. L., Hou, L. G.
core +1 more source
Testing Yukawa cosmology at the Milky Way and M31 galactic scales [PDF]
We address the galaxy rotation curves through the Yukawa gravitational potential emerging as a correction of the Newtonian potential in extended theories of gravity.
R. D’Agostino +2 more
semanticscholar +1 more source
The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream [PDF]
It has recently been shown that the Large Magellanic Cloud (LMC) has a substantial effect on the Milky Way’s stellar halo and stellar streams. Here, we explore how deformations of the Milky Way and LMC’s dark matter haloes affect stellar streams, and ...
Sophia Lilleengen +15 more
semanticscholar +1 more source
What Does the Milky Way Look Like?
In spite of much work, the overall spiral structure morphology of the Milky Way remains somewhat uncertain. In the last two decades, accurate distance measurements have provided us with an opportunity to solve this issue.
Y. Xu +7 more
doaj +1 more source
Cosmological Structures behind the Milky Way
This paper provides an update to the review on extragalactic large-scale structures uncovered in the Zone of Avoidance (ZOA) by Kraan-Korteweg & Lahav 2000, in particular in the Great Attractor region. Emphasis is given to the penetration of the ZOA with
Kraan-Korteweg, Renee C.
core +1 more source

