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Related papers: Dynamics of Mergers

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Recent results are reviewed on galaxy dynamics, bar evolution, destruction and re-formation, cold gas accretion, gas radial flows and AGN fueling, minor mergers. Some problems of galaxy evolution are discussed in particular, exchange of…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 Francoise Combes

I will try to put the ultraluminous galaxy phenomenon into a broad cosmological context. Viewed from this perspective, the significance of ultraluminous galaxies and the `starburst vs. monster' debate becomes clear. Ultraluminous galaxies…

Astrophysics · Physics 2007-05-23 Timothy M. Heckman

Galaxy mergers are hugely important in our current dark matter cosmology. These powerful events cause the disruption of the merging galaxies, pushing the gas, stars and dust of the galaxies resulting in changes to morphologies. This…

Astrophysics of Galaxies · Physics 2023-02-23 W. J. Pearson , L. E. Suelves , S. C. -C. Ho , N. Oi , NEP Team , GAMA Team

This chapter reviews how galactic inflows influence galaxy metallicity. The goal is to discuss predictions from theoretical models, but particular emphasis is placed on the insights that result from using models to interpret observations.…

Astrophysics of Galaxies · Physics 2017-05-31 Kristian Finlator

In this review we discuss the evidence for galaxy interactions and mergers in the distant universe and the role of mergers in forming galaxies. Observations show that the fraction of massive (M> M_*) galaxies involved in major mergers is…

Astrophysics · Physics 2009-11-11 Christopher J. Conselice

Most luminous infrared galaxies (LIGs) are closely interacting/merging systems rich in molecular gas. We study here the relationship between the stage of the galaxy-galaxy interactions, the molecular gas mass, and the star formation rate as…

Astrophysics · Physics 2016-08-30 Yu Gao , Philip M. Solomon

We numerically investigate dynamical and chemical properties of star clusters (open and globular clusters, and ``super star clusters'', SSC) formed in interacting/merging galaxies. The investigation is two-fold: (1) large-scale…

Astrophysics · Physics 2009-11-10 Kenji Bekki

Several simple mergers between model galaxy clusters containing a mixture of gas and dark matter are examined, testing the coupling of the gas to the underlying collisionless material. The gas is shocked, irreversibly dissipating the energy…

Astrophysics · Physics 2015-06-24 F. R. Pearce , P. A. Thomas , H. M. P. Couchman

We study the gravitational stability of gaseous streams in the complex environment of a galaxy merger, because mergers are known to be places of ongoing massive cluster formation and bursts of star formation. We find an analytic stability…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Andres Escala , Fernando Becerra , Luciano del Valle , Esteban Castillo

A review of gravitational and hydrodynamical processes during formation of clusters and evolution of galaxies is given. Early, at the advent of N-body computer simulations, the importance of tidal fields in galaxy encounters has been…

Astrophysics · Physics 2015-06-24 Jan Palous

We report mid-infrared observations of several luminous infrared galaxies (LIGs) carried out with the Infrared Space Observatory. Our sample was chosen to represent different phases of a merger sequence of galaxy-galaxy interaction with…

Astrophysics · Physics 2015-06-24 Chorng-Yuan Hwang , K. Y. Lo , Yu Gao , Robert A. Gruendl , Nanyao Y. Lu

Theoretical considerations and observational data support the idea that mergers were more frequent in the past. At high redshifts, violent interactions and mergers may be implicated in the origin of Lyman-break galaxies, sub-mm starbursts,…

Astrophysics · Physics 2007-05-23 Joshua E. Barnes

Asymmetries in galactic potentials, either self-induced, or caused by a passing companion, play an important role in global gas dynamics in galaxies. In particular, they are able to trigger gas inflow, which in turn feeds nuclear activity.…

Astrophysics · Physics 2007-05-23 Witold Maciejewski

Central regions of superclusters are the ideal places where to study cluster merging phenomena: in fact the accretion activity is enhanced, as predicted by the cosmological simulations. In this paper I review the case-study of the Shapley…

Astrophysics · Physics 2009-11-10 S. Bardelli

Galaxy mergers have been shown to trigger AGN in the nearby universe, but the timescale over which this process happens remains unconstrained. The Multi-Model Merger Identifier (MUMMI) machine vision pipeline has been demonstrated to…

We present a brief overview of some recent observations of colliding galaxies and relevant numerical simulations. These are compared, and details of the locations and history of collision induced star formation are explored, with possible…

Astrophysics · Physics 2007-05-23 Susan A. Lamb , Nathan C. Hearn

Recent work on the dynamical evolution of galactic nuclei containing supermassive black holes is reviewed. Topics include galaxy structural properties; collisionless and collisional equilibria; loss-cone dynamics; and dynamics of binary and…

Astrophysics · Physics 2009-11-11 David Merritt

During the merger of two galaxies, the resulting system undergoes violent relaxation and seeks stable equilibrium. However, the details of this evolution are not fully understood. Using Illustris simulation, we probe two physically related…

Astrophysics of Galaxies · Physics 2018-02-28 Anthony M. Young , Liliya L. R. Williams , Jens Hjorth

The study of colliding galaxies has progressed rapidly in the last few years, driven by observations with powerful new ground and space-based instruments. These instruments have used for detailed studies of specific nearby systems,…

Astrophysics · Physics 2015-06-24 Curtis Struck

Galaxy merger simulations have explored the behaviour of gas within the galactic disk, yet the dynamics of hot gas within the galaxy halo has been neglected. We report on the results of high-resolution hydrodynamic simulations of colliding…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 Manodeep Sinha , Kelly Holley-Bockelmann
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