Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

GASTRO Library. II. Exploring Chemical Bimodalities in Disk Galaxies with GSE-like Mergers and Massive Star-forming Clumps

  • Authors: João A. S. Amarante, Chervin F. P. Laporte, Victor P. Debattista, Leandro Beraldo e Silva, Guilherme Limberg, Hélio D. Perottoni, Zhao-Yu Li, Lais Borbolato, Karl Fiteni, Chengye Cao, Nathan Deg, Tigran Khachaturyants, Xiaojie Liao

João A. S. Amarante et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure B1.

[O/Fe] histogram for the interval −0.7 < [Fe/H] < − 0.2, 4 < R/kpc < 12, and ∣z∣ < 3 kpc. The dark and light-shaded areas correspond to the contribution of stars born in the inner part of the galaxy, i.e., R  <  4 kpc, with orbital circularity ηs < 0.9 and ηs > 0.9, respectively. Overall, from the stars born in the inner part of the galaxy that contribute to the α-rich peak at the disk, there is a larger fraction with hotter orbits in the clumpy models.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse