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The evolution of our Universe is strongly influenced by the attractive force of gravity. A key aspect of this evolution, therefore, is the merging of galaxies. Here, we explore the role of mergers in shaping the properties of massive…

星系天体物理 · 物理学 2025-06-12 Sugata Kaviraj

The importance of the post-merger epoch in galaxy evolution has been well-documented, but post-mergers are notoriously difficult to identify. While the features induced by mergers can sometimes be distinctive, they are frequently missed by…

Galaxy mergers are known to trigger bursts of central star formation, which should therefore lead to stellar mass growth in their inner regions. However, observational measurements of this `burst mass fraction' are scant. Here, we assemble…

星系天体物理 · 物理学 2026-04-27 Sara L. Ellison , Leonardo Ferreira

Galaxies are surrounded by sizeable gas reservoirs which host a significant amount of metals: the circum-galactic medium (CGM). The CGM acts as a mediator between the galaxy and the extra-galactic medium. However, our understanding of how…

星系天体物理 · 物理学 2018-01-22 Maan H. Hani , Martin Sparre , Sara L. Ellison , Paul Torrey , Mark Vogelsberger

The dynamical history of most merging galaxies is not well understood. Correlations between galaxy interaction and star formation have been found in previous studies, but require the context of the physical history of merging systems for…

Various galaxy merger detection methods have been applied to diverse datasets. However, it is difficult to understand how they compare. We aim to benchmark the relative performance of machine learning (ML) merger detection methods. We…

Galaxy mergers play a crucial role in shaping the morphology, the star formation, and the mass growth of galaxies across cosmic time. While mergers have been extensively investigated in the local Universe, the evolution of their frequency…

Aims. We aim to perform consistent comparisons between observations and simulations on the mass dependence of the galaxy major merger fraction at low redshift over an unprecedentedly wide range of stellar masses (10^9 to 10^12 solar…

星系天体物理 · 物理学 2021-01-04 L. Wang , W. J. Pearson , V. Rodriguez-Gomez

The process of galaxy evolution over cosmic time is not yet fully understood, since there is a debate on the impact of galaxy collisions on the star formation and metallicity. The local environment of the galaxy mergers could also have a…

星系天体物理 · 物理学 2025-09-12 Bendeguz Koncz , Istvan Horvath , András Péter Joó , Andreas Burkert , L. Viktor Tóth

The role of major mergers in galaxy and black hole formation is not well constrained. To help address this, we develop an automated method to identify late-stage galaxy mergers before coalescence of the galactic cores. The resulting sample…

We present a study of galaxy mergers up to $z=10$ using the Planck Millennium cosmological dark matter simulation and the {\tt GALFORM} semi-analytical model of galaxy formation. Utilising the full ($800$ Mpc)$^3$ volume of the simulation,…

星系天体物理 · 物理学 2021-12-17 Filip Huško , Cedric G. Lacey , Carlton M. Baugh

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…

星系天体物理 · 物理学 2023-02-23 W. J. Pearson , L. E. Suelves , S. C. -C. Ho , N. Oi , NEP Team , GAMA Team

Galaxy merging is the late time manifestation of the galaxy formation process and likely significantly effects $z<1$ galaxies. A ``maximum reasonable rate'' model for merging finds a $\sim2$ mag K band increase in the luminosities of dwarf…

天体物理学 · 物理学 2016-08-30 R. G. Carlberg

We derive the number of dynamically close companions per galaxy ($N_c$) and their total luminosity ($L_c$) for galaxies in the Millennium Galaxy Catalogue: $N_c$ is similar to the fraction of galaxies in close pairs and is directly related…

天体物理学 · 物理学 2008-11-26 R. De Propris , J. Liske , S. P. Driver , P. Allen , N. J. G. Cross

Galaxy mergers are expected to have a profound influence on the star formation histories of galaxies. It is generally expected that mergers are the main drivers of galaxy mass growth through the accretion of mass and the triggering of new…

星系天体物理 · 物理学 2026-02-18 Josephine Chishala , Roberto De Propris , Mirjana Pović

Clusters of galaxies are merging during the formation of large-scale structures in the Universe. Based on optical survey data, we identify a large sample of pre-mergers of galaxy clusters and merging subclusters in rich clusters. We find…

宇宙学与河外天体物理 · 物理学 2024-06-04 Z. L. Wen , J. L. Han , Z. S. Yuan

Mergers of galaxies are extremely violent events shaping their evolution. Such events are thought to trigger starbursts and, possibly, black hole accretion. Nonetheless, it is still not clear how to know the fate of a galaxy pair from the…

星系天体物理 · 物理学 2020-02-05 Hugo Pfister , Massimo Dotti , Clothilde Laigle , Yohan Dubois , Marta Volonteri

A key obstacle to understanding the galaxy merger rate and its role in galaxy evolution is the difficulty in constraining the merger properties and time-scales from instantaneous snapshots of the real universe.The most common way to…

天体物理学 · 物理学 2009-11-13 Jennifer M. Lotz , Patrik Jonsson , T. J. Cox , Joel R. Primack

Galaxy mergers are fundamental drivers of galaxy evolution and black hole (BH) growth across cosmic time. We use the Horizon-AGN simulation to investigate the fraction of galaxy pairs, the merger fraction, and the galaxy merger rate over a…

星系天体物理 · 物理学 2026-05-14 Ecaterina Leonova , Marta Volonteri , Clotilde Laigle , Samaya Nissanke , Pascal A. Oesch , Yohan Dubois