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Astrophysical tests of dark matter self-interactions

Reviews of Modern Physics, 2022
Self-interacting dark matter (SIDM) arises generically in scenarios for physics beyond the Standard Model that have dark sectors with light mediators or strong dynamics.
S. Adhikari   +13 more
semanticscholar   +1 more source

Galaxies in Interaction

Astronomische Nachrichten, 2004
AbstractPosters: Because of the large number of contributions, some oral presentations had to be transferred into Posters. The reader is referred to the final programme for the actual allocation of Posters.A01 Chemical Enrichment of the Intracluster MediumA02 Structural analysis of high‐velocity clouds – Evidence for an interaction between the Milky ...
Hüttemeister, Susanne   +2 more
openaire   +1 more source

Gravitational Interactions between Galaxies

Symposium - International Astronomical Union, 1974
Recent theoretical studies of the consequences of fierce tidal interactions between galaxies are reviewed and compared.
openaire   +1 more source

Dynamics of Interacting Galaxies

Annual Review of Astronomy and Astrophysics, 1992
The dynamics of interacting galaxies as observed in the present epoch is reviewed. Topics discussed include numerical methods for modeling galactic interactions, the signatures of interacting galaxies due to tidal forces, and events that add mass to a galaxy.
Joshua E. Barnes, Lars Hernquist
openaire   +2 more sources

Gravitational interactions between galaxies

Physics Reports, 1982
Abstract The dynamics of an encounter between two galaxies is discussed. Generally in galactic encounter, on account of the tidal forces, the binding energies of the galaxies increase and hence their relative orbital energy decreases. The former has disruptive effects on galaxies and the latter may lead to the merging of galaxies under certain ...
Saleh Mohammed Alladin   +1 more
openaire   +1 more source

Interactions between Galaxies

1995
Gravitational interactions between galaxies are far more common than one might think, assuming that the space density of galaxies is uniform. The galaxies in effect group themselves in clusters, small groups, or pairs: far from being isolated systems they are formed and evolve in interaction with their environment and in particular with neighbouring ...
Françoise Combes   +3 more
openaire   +1 more source

Galaxy Interactions and the Radio Galaxy Phenomenon

1990
We have been studying powerful radio galaxies (which we define as having radio power at 178MHz, P 178 ≥ 5xl024 Watts/Hz for a cosmology of H o = 100 km sec-1 Mpc-1 and q o = 0) in order to determine their origins. There are two distinct classes of powerful radio galaxies (PRGs), the so called class A and B radio galaxies (Hine and Longair 1979; Heckman
E. P. Smith, T. M. Heckman
openaire   +1 more source

Bar Formation by Galaxy-Galaxy Interactions

2004
Bar formation process in interacting galaxies is reviewed on the basis of recent numerical simulations. I focus especially on the possible kinematical difference between tidally-induced bars and spontaneous bars: the former spans a wider range in the rotation rate, depending upon the parameters of the interaction as well as the internal structure of ...
openaire   +1 more source

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