Adaptive mesh refinement simulations of collisional ring galaxies: effects of the interaction geometry

Author:

Fiacconi Davide1,Mapelli Michela2,Ripamonti Emanuele1,Colpi Monica1

Affiliation:

1. Dipartimento di Fisica ‘G. Occhialini’; Università di Milano-Bicocca; Piazza della Scienza 3; I-20126; Milano; Italy

2. INAF-Osservatorio Astronomico di Padova; Vicolo dell'Osservatorio 5; I-35122; Padova; Italy

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 19 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Formation of collisional ring galaxies in Milgromian dynamics;Monthly Notices of the Royal Astronomical Society;2024-01-08

2. Do ultra diffuse galaxies with rich globular clusters systems have overly massive haloes?;Monthly Notices of the Royal Astronomical Society;2023-12-30

3. A giant umbrella-like stellar stream around the tidal ring galaxy NGC 922;Astronomy & Astrophysics;2023-01

4. The peculiar galaxy HRG 705: A possible on-going merging?;Monthly Notices of the Royal Astronomical Society;2022-06-24

5. Differences in star formation activity between tidally triggered and isolated bars: a case study of NGC 4303 and NGC 3627;Monthly Notices of the Royal Astronomical Society;2021-11-25

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