Phylogeny of the Milky Way’s inner disk and bulge populations: Implications for 
gas accretion, (the lack of) inside-out thick disk formation and quenching

Haywood, Misha; Matteo, Paola Di; Lehnert, Matthew; Snaith, Owain; Fragkoudi, Francesca; Khoperskov, Sergey

doi:10.1051/0004-6361/201731363

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Phylogeny of the Milky Way’s inner disk and bulge populations: Implications for gas accretion, (the lack of) inside-out thick disk formation and quenching

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Fragkoudi, Francesca
Computational Structure Formation, MPI for Astrophysics, Max Planck Society;

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Haywood, M., Matteo, P. D., Lehnert, M., Snaith, O., Fragkoudi, F., & Khoperskov, S. (2018). Phylogeny of the Milky Way’s inner disk and bulge populations: Implications for gas accretion, (the lack of) inside-out thick disk formation and quenching. Astronomy and Astrophysics, 618: A78, pp. 1-23. doi:10.1051/0004-6361/201731363.

Cite as: https://hdl.handle.net/21.11116/0000-0003-1858-0

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