Two chemically similar stellar overdensities on opposite sides of the plane of the Galactic disk
<p>Our Galaxy is thought to have undergone an active evolutionary history dominated by star formation, the accretion of cold gas, and, in particular, mergers up to 10 gigayear ago. The stellar halo reveals rich fossil evidence of these interactions in the form of stellar streams, substructures...
Κύριοι συγγραφείς: | Bergemann, M, Sesar, B, Cohen, J, Serenelli, A, Sheffield, A, Li, T, Casagrande, L, Johnston, K, Laporte, C, Price-Whelan, A, Schönrich, R, Gould, A |
---|---|
Μορφή: | Journal article |
Γλώσσα: | English |
Έκδοση: |
Nature Publishing Group
2018
|
Παρόμοια τεκμήρια
Παρόμοια τεκμήρια
-
Properties of Stellar Streams in the Galactic Disk
ανά: Marsakov V. A., κ.ά.
Έκδοση: (2016-12-01) -
All-sky Kinematics and Chemistry of Monoceros Stellar Overdensity
ανά: Lais Borbolato, κ.ά.
Έκδοση: (2023-01-01) -
STELLAR DISTRIBUTION-FUNCTIONS FOR GALACTIC DISKS
ανά: Villumsen, J, κ.ά.
Έκδοση: (1985) -
A project for investigation of stellar population of the galactic disk
ανά: Straižys V., κ.ά.
Έκδοση: (1994-03-01) -
Non-local thermodynamic equilibrium stellar spectroscopy with 1D and 〈3D〉 models. II. Chemical properties of the galactic metal-poor disk and the halo
ανά: Bergemann, M, κ.ά.
Έκδοση: (2017)