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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

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.

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Item Permalink: http://hdl.handle.net/21.11116/0000-0003-1858-0 Version Permalink: http://hdl.handle.net/21.11116/0000-0003-1859-F
Genre: Journal Article

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 Creators:
Haywood, Misha, Author
Matteo, Paola Di, Author
Lehnert, Matthew, Author
Snaith, Owain, Author
Fragkoudi, Francesca1, Author              
Khoperskov, Sergey, Author
Affiliations:
1Computational Structure Formation, MPI for Astrophysics, Max Planck Society, ou_2205642              

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 Dates: 2018-10-16
 Publication Status: Published online
 Pages: -
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 Rev. Method: -
 Identifiers: DOI: 10.1051/0004-6361/201731363
Other: LOCALID: 3030787
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Title: Astronomy and Astrophysics
  Other : Astron. Astrophys.
Source Genre: Journal
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Publ. Info: France : EDP Sciences S A
Pages: - Volume / Issue: 618 Sequence Number: A78 Start / End Page: 1 - 23 Identifier: ISSN: 1432-0746
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1