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相关论文: Ultraluminous Starbursts in Major Mergers

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Using numerical simulation, we study the development of gaseous inflows and triggering of starburst activity in mergers of comparable-mass disk galaxies. In all encounters studied, the galaxies experience strong gaseous inflows and moderate…

天体物理学 · 物理学 2009-10-28 Chris Mihos , Lars Hernquist

Extragalactic starbursts induced by gravitational interactions can now be studied from z = ~0 to ~2. The evidence that mergers of gas-rich galaxies tend to trigger galaxy-wide starbursts is strong, both statistically and in individual cases…

天体物理学 · 物理学 2015-11-11 Francois Schweizer

Galaxy interactions and mergers play a significant, but still debated and poorly understood role in the star formation history of galaxies. Numerical and theoretical models cannot yet explain the main properties of merger-induced…

宇宙学与河外天体物理 · 物理学 2015-05-20 Frederic Bournaud , Leila C. Powell , Damien Chapon , Romain Teyssier

There is increasing evidence for the presence of blue super star clusters in the central regions of ultraluminous infrared galaxies like Arp 220. Ultraluminous galaxies are thought to be triggered by galaxy mergers, and it has often been…

天体物理学 · 物理学 2009-10-30 Yoshiaki Taniguchi , Neil Trentham , Yasuhiro Shioya

We study the shape and evolution of the star formation main sequence in three independently developed semi-analytic models of galaxy formation. We focus, in particular, on the characterization of the model galaxies that are significantly…

星系天体物理 · 物理学 2019-03-15 Lan Wang , Gabriella De Lucia , Fabio Fontanot , Michaela Hirschmann

The correspondence between galaxy major mergers and starburst activity is well-established observationally and in simulations of low redshift galaxies. However, the evolution of the properties of interactions and of the galaxies involved…

星系天体物理 · 物理学 2022-09-21 Florent Renaud , Álvaro Segovia Otero , Oscar Agertz

We present hydrodynamic simulations of a major merger of disk galaxies, and study the ISM dynamics and star formation properties. High spatial and mass resolutions of 12pc and 4x10^4 M_sol allow to resolve cold and turbulent gas clouds…

宇宙学与河外天体物理 · 物理学 2015-05-19 Romain Teyssier , Damien Chapon , Frederic Bournaud

The most active starbursts are found in galaxies with the highest IR luminosities, with peak star formation rates and efficiencies that are over an order of magnitude higher than in normal disk systems. These systems are almost exclusively…

天体物理学 · 物理学 2009-10-30 J. E. Hibbard

Major mergers and interactions between gas-rich galaxies with comparable masses are thought to be the main triggers of starburst. In this work, we study, for a large stellar mass range, the interaction rate of the starburst galaxies in the…

星系天体物理 · 物理学 2015-06-22 Wentao Luo , Xiaohu Yang , Youcai Zhang

We investigate the relative importance of starbursts and AGN in nuclear activities of ultra-luminous infrared galaxies (ULIRGs) based on chemodynamical simulations combined with spectrophotometric synthesis codes. We numerically investigate…

天体物理学 · 物理学 2009-11-11 Kenji Bekki , Yashuhiro Shioya , Matthew Whiting

We use cosmological SPH simulations to study the effects of mergers in the star formation history of galactic objects in hierarchical clustering scenarios. We find that during some merger events, gaseous discs can experience two starbursts:…

天体物理学 · 物理学 2009-11-07 P. B. Tissera , R. Dominguez-Tenreiro , C. Scannapieco , A. Saiz

It has been often considered that the dissipative collapse caused by a merger of two gas-rich galaxies is responsible for the intense nuclear starbursts or the nonthermal quasar activity in ultraluminous infrared galaxies due to the…

天体物理学 · 物理学 2009-10-30 Yoshiaki Taniguchi , Yasuhiro Shioya

Starburst (SB) galaxies are a rare population of galaxies with star formation rates (SFRs) greatly exceeding those of the majority of star-forming galaxies with similar stellar mass. It is unclear whether these bursts are the result of…

星系天体物理 · 物理学 2023-09-19 Elia Cenci , Robert Feldmann , Jindra Gensior , Jorge Moreno , Luigi Bassini , Mauro Bernardini

We numerically investigate stellar and gaseous dynamical evolution of mergers between five identical late-type disk galaxies with the special emphasis on star formation history and chemical evolution of multiple galaxy mergers. We found…

天体物理学 · 物理学 2009-10-31 Kenji Bekki

The extraordinary starbursts found in ultraluminous IR galaxies occur in molecular gas concentrated in compact very massive "clouds" which we call "Extreme Starbursts". They have one thousand times the mass but are only a few times larger…

天体物理学 · 物理学 2007-05-23 P. M. Solomon

We introduce the `Illustris zoom simulation project', which allows the study of selected galaxies forming in the $\Lambda$CDM cosmology with a 40 times better mass resolution than in the parent large-scale hydrodynamical Illustris…

星系天体物理 · 物理学 2016-08-01 Martin Sparre , Volker Springel

Recent simulation work has successfully captured the formation of the star clusters that have been observed in merging galaxies. These studies, however, tend to focus on studying extreme starbursts, such as the Antennae galaxies. We aim to…

宇宙学与河外天体物理 · 物理学 2015-06-16 Leila C. Powell , Frederic Bournaud , Damien Chapon , Romain Teyssier

We propose that synchronized triggering of star formation in gas-rich galaxies is possible during major mergers of cluster of galaxies, based on new numerical simulations of the time evolution of the physical properties of the intracluster…

宇宙学与河外天体物理 · 物理学 2015-05-19 Kenji Bekki , Matt S. Owers , Warrick J. Couch

Ultraluminous infrared galaxies (ULIRGs) with multiple ($\ge 3$) nuclei are frequently observed. It has been suggested that these nuclei are produced by multiple major mergers of galaxies. The expected rate of such mergers is, however, too…

There is a consensus in the literature that starburst galaxies are triggered by inter- action events. However, it remains an open question as to what extent both merging and non-merging interactions have in triggering starbursts? In this…

星系天体物理 · 物理学 2018-06-13 C. L. Wilkinson , K. A. Pimbblet , J. P. Stott , C. G. Few , B. K. Gibson
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