The Imprint of Clump Formation at High Redshift. II. The Chemistry of the Bulge

The Imprint of Clump Formation at High Redshift. II. The Chemistry of the Bulge

In Paper I, we showed that clumps in high-redshift galaxies, having a high star formation rate density (Σ _SFR ), produce disks with two tracks in the [Fe/H]–[ α /Fe] chemical space, similar to that of the Milky Way’s (MW’s) thin+thick disks. Here we investigate the effect of clumps on the bulge’s c...

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Bibliographic Details
Main Authors: Victor P. Debattista, David J. Liddicott, Oscar A. Gonzalez, Leandro Beraldo e Silva, João A. S. Amarante, Ilin Lazar, Manuela Zoccali, Elena Valenti, Deanne B. Fisher, Tigran Khachaturyants, David L. Nidever, Thomas R. Quinn, Min Du, Susan Kassin
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Galactic bulge
Milky Way formation
Milky Way evolution
Milky Way dynamics
Galaxy bulges
Online Access:https://doi.org/10.3847/1538-4357/acbb00

Internet

https://doi.org/10.3847/1538-4357/acbb00

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