Articles citing this article

The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).

Cited article:

Forming disk galaxies in major mergers - II. The central mass concentration problem and a comparison of GADGET3 with GIZMO

S. A. Rodionov, E. Athanassoula, N. Peschken

A&A, 600 (2017) A25

Published online: 2017-03-22

DOI: https://doi.org/10.1051/0004-6361/201628319

This article has been cited by the following article(s):

The origin of metal-poor stars on prograde disc orbits in FIRE simulations of Milky Way-mass galaxies

Isaiah B Santistevan, Andrew Wetzel, Robyn E Sanderson, et al.
Monthly Notices of the Royal Astronomical Society 505 (1) 921 (2021)
https://doi.org/10.1093/mnras/stab1345

Disc galaxies formed from major mergers in Illustris

E Athanassoula, Ewa L Łokas and Nicolas Peschken
Monthly Notices of the Royal Astronomical Society 493 (1) 1375 (2020)
https://doi.org/10.1093/mnras/staa299

Linking bar- and interaction-driven molecular gas concentration with centrally enhanced star formation in EDGE–CALIFA galaxies

Ryan Chown, Cheng Li, E Athanassoula, et al.
Monthly Notices of the Royal Astronomical Society 484 (4) 5192 (2019)
https://doi.org/10.1093/mnras/stz349

External versus internal triggers of bar formation in cosmological zoom-in simulations

Tommaso Zana, Massimo Dotti, Pedro R. Capelo, et al.
Monthly Notices of the Royal Astronomical Society 473 (2) 2608 (2018)
https://doi.org/10.1093/mnras/stx2503

Evolution of the anti-truncated stellar profiles of S0 galaxies since z = 0.6 in the SHARDS survey

Alejandro Borlaff, M. Carmen Eliche-Moral, John E. Beckman, et al.
Astronomy & Astrophysics 615 A26 (2018)
https://doi.org/10.1051/0004-6361/201732090

Using N-body simulations to understand the chemo-dynamical evolution of the inner Milky Way

E. Athanassoula
Proceedings of the International Astronomical Union 13 (S334) 65 (2017)
https://doi.org/10.1017/S1743921317008778