A dynamically young and perturbed Milky Way disk
T Antoja, A Helmi, M Romero-Gómez, D Katz… - Nature, 2018 - nature.com
The evolution of the Milky Way disk, which contains most of the stars in the Galaxy, is
affected by several phenomena. For example, the bar and the spiral arms of the Milky Way …
affected by several phenomena. For example, the bar and the spiral arms of the Milky Way …
Two chemically similar stellar overdensities on opposite sides of the plane of the Galactic disk
M Bergemann, B Sesar, JG Cohen, AM Serenelli… - Nature, 2018 - nature.com
Our Galaxy is thought to have an active evolutionary history, dominated over the past ten
billion years or so by star formation, the accretion of cold gas and, in particular, the merging …
billion years or so by star formation, the accretion of cold gas and, in particular, the merging …
6. Phenomenology and Physics of Late-Type Stars
M BERGEMANN, CJ HANSEN… - Radiative Transfer in …, 2020 - books.google.com
In this chapter, we present the basics of the physics and phenomenology of FGKM-type
stars. This review is based on recent developments in the observational and theoretical …
stars. This review is based on recent developments in the observational and theoretical …
Two chemically similar stellar overdensities on opposite sides of the plane of the Galaxy
M Bergemann, B Sesar, JG Cohen… - arXiv preprint arXiv …, 2018 - arxiv.org
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 …
formation, the accretion of cold gas, and, in particular, mergers up to 10 gigayear ago. The …
Riding the waves: The formation and evolution of vertical bending waves in Milky Way-like disc galaxies
MH Chequers - 2018 - search.proquest.com
In this thesis we study the dynamics of vertical (bending) waves in Milky Way-like disc
galaxies. The main goals of the thesis are to form a coherent picture for the formation and …
galaxies. The main goals of the thesis are to form a coherent picture for the formation and …