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Abundance Gradients as a tool for understanding the Formation of the Milky Way
Astrophysics and Space Science, 2002According to the two-infall model for the chemical evolution of the Galaxy (Chiappini et al., 2001) the halo and bulge formed on a relatively short timescale (0.8–1.0 Gyr) out of the first infall episode, whereas the disk accumulated much more slowly and ‘inside-out’ during a second independent infall episode.
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Abundance Ratios and the Formation of the Milky Way
2006Although the data for the Milky Way are not yet conclusive about the existence of a N/O abundance gradient along the Galactic disk, such a gradient is clearly seen in other spiral galaxies [7]. In this work we computed the abundance gradient of N/O for the MW. In our formalist the MW formed out of two-infall episodes, one forming the halo/thick disk on
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Self-Interacting Dark Matter Subhalos in the Milky Way’s Tides
Physical Review Letters, 2020Laura V Sales, Hai-Bo Yu, Omid Sameie
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High-Mass Star and Massive Cluster Formation in the Milky Way
Annual Review of Astronomy and Astrophysics, 2018Frédérique Motte
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Debris streams in the solar neighbourhood as relicts from the formation of the Milky Way
Nature, 1999Hongsheng Zhao, Simon White
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Star Formation in the Milky Way and Nearby Galaxies
Annual Review of Astronomy and Astrophysics, 2012Neal Evans, Robert Kennicutt
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Galactic Structure Surveys and the Evolution of the Milky Way
Annual Review of Astronomy and Astrophysics, 1993S R Majewski
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