Results 61 to 70 of about 8,688,256 (155)
The main-sequence turnoff (MSTO) stars well preserve the chemical properties where they were born, making them ideal tracers for studying the stellar population. We perform a detailed chemo-dynamical analysis on moderately metal-poor (−2.0
Renjing Xie +7 more
doaj +1 more source
Disentangling the Distant Stellar Halo Using K Giants in DESI Year 3 Data
We present a sample of 88,959 K giants from Dark Energy Spectroscopic Instrument Milky Way Survey Year 3 data, which we use to characterize the chemo-dynamical properties of the stellar halo at Galactocentric distances of 12 to ∼100 kpc.
Namitha Kizhuprakkat +44 more
doaj +1 more source
Python code that implements the dark matter halo contraction given in Cautun et al (2020) and the best fitting Milky Way mass profile given the latest Gaia DR2 rotation curve of our ...
Thomas M. Callingham, Marius Cautun
core +1 more source
The Extremely Metal-rich Knot of Stars at the Heart of the Galaxy
We show with Gaia XP spectroscopy that extremely metal-rich (EMR) stars in the Milky Way ([M/H] _XP ≳ 0.5) are largely confined to a tight “knot” at the center of the Galaxy. This EMR knot is round in projection, has a fairly abrupt edge near R _GC,proj ∼
Hans-Walter Rix +17 more
doaj +1 more source
Dynamics and history of the Milky Way
Our understanding of the Milky Way and its constituents is undergoing a revolutionary change driven primarily by the Gaia space mission, and which is further reinforced when combined with spectroscopic surveys from the ground.
Helmi, Amina
core
Measuring the Milky Way Vertical Potential with the Phase Snail in a Model-independent Way
The vertical phase-space spiral (snail) is a direct sign of disequilibrium of the Milky Way’s disk. Nevertheless, the wrapping of the phase snail contains information on the vertical potential.
Rui Guo +4 more
doaj +1 more source
Recent measurements of the Milky Way rotation curve found a sharp decline at around 15–20 kpc from the center of the Galaxy, suggesting that the Galactic dark matter halo is much less massive than predicted by other dynamical tracers.
Xiaowei Ou +5 more
doaj +1 more source
In this article, I describe constructing a scale model of our galaxy—the Milky Way—and using this model to teach modern astronomy. The Milky Way model expands on concepts usually explored in the more common solar system model.
Friedman, Robert B.
core
Milky Way versus Andromeda: a tale of two disks
Aims. We study the chemical evolution of the disks of the Milky Way (MW) and of Andromeda (M31), to identify the common properties and differences between the two major galaxies of the Local ...
J. L. Hou +13 more
core +1 more source

