Popping star clusters as building blocks of the Milky Way’s thick disc
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/415/2/1280/3495007/mnras0415-1280.pdf
Reference33 articles.
1. Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. II. The Fine Structure of Simulated Galactic Disks
2. Chemical similarities between Galactic bulge and local thick disk red giants: O, Na, Mg, Al, Si, Ca, and Ti
3. The Accretion Origin of the Milky Way’s Stellar Halo
4. Elemental abundance trends in the Galactic thin and thick disks as traced by nearby F and G dwarf stars
5. Tracing the Galactic Thick Disk to Solar Metallicities
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1. The Physical Thickness of Stellar Disks to z ∼ 2;The Astrophysical Journal;2023-10-01
2. The escape of globular clusters from the satellite dwarf galaxies of the Milky Way;Monthly Notices of the Royal Astronomical Society;2022-04-20
3. Bimodality of [α Fe]–[Fe/H] distributions is a natural outcome of dissipative collapse and disc growth in Milky Way-type galaxies;Monthly Notices of the Royal Astronomical Society;2021-01-15
4. A Dynamical Model for Clustered Star Formation in the Galactic Disk;The Astrophysical Journal;2019-10-23
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