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Related papers: Starbursts and the Evolution of Gas-Rich Galaxies

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The rate of star formation varies between galaxy types and evolves with redshift. Most stars in the universe have formed in episodes of an exceptionally high star-forming activity, commonly called a starburst. We here summarize basic…

Astrophysics of Galaxies · Physics 2020-12-24 Ivana Orlitova

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…

Astrophysics · Physics 2007-05-23 P. M. Solomon

Starbursts are extreme concentrations of star-forming activity with mass conversion surface densities reaching over 1000 times higher than normal for disk galaxies. They are responsible for a large fraction of all cosmic star formation.…

Astrophysics · Physics 2007-05-23 Robert W. O'Connell

I review the properties of starburst galaxies in the nearby and distant universe to decipher their evolution as a distinct extragalactic class. The physical processes and environments of massive star-formation appear to be similar out to z…

Astrophysics · Physics 2007-05-23 Christopher J. Conselice

Low-mass disk galaxies with well-organized structures are relatively common in low density regions of the nearby Universe. They display a wide range in levels of star formation activity, extending from sluggishly evolving `superthin' disk…

Astrophysics · Physics 2007-05-23 J. S. Gallagher , L. D. Matthews

Starbursts are episodes of intense star-formation that occur in the central regions of galaxies, and dominate the integrated emission from the galaxy. They are a significant component of the present- day universe, being the site of $\sim$…

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

Observations of intensely bright star-forming galaxies both close by and in the distant Universe at first glance seem to emphasize their similarity. But look a little closer, and differences emerge.

Cosmology and Nongalactic Astrophysics · Physics 2015-05-18 Yu Gao

Using parsec-resolution simulations of a typical galaxy merger, we study the triggering of starbursts by connecting the (inter-)galactic dynamics to the structure of the interstellar medium. The gravitational encounter between two galaxies…

Astrophysics of Galaxies · Physics 2015-06-19 Florent Renaud , Frédéric Bournaud , Katarina Kraljic , Pierre-Alain Duc

Nearby (D < 100 Mpc) luminous blue starburst galaxies frequently show morphological evidence for recent involvement in mild collisions, or minor mergers where the disk survives. As a consequence UV-bright starbursts are preferentially seen…

Star-formation and the Starburst phenomenon are presented with respect to a number of nearby star-forming galaxies where our understanding of the process can be calibrated. Methods of estimating star-formation rates are discussed together…

Astrophysics · Physics 2007-05-23 T. W. B. Muxlow , R. J. Beswick , A. M. S. Richards , H. Thrall

Young galaxies are clumpy, gas-rich, and highly turbulent. Star formation appears to occur by gravitational instabilities in galactic disks. The high dispersion makes the clumps massive and the disks thick. The star formation rate should be…

Astrophysics of Galaxies · Physics 2015-05-27 Bruce G. Elmegreen

Starbursts are episodes of intense star-formation in the central regions of galaxies, and are the sites of roughly 25% of the high-mass star-formation in the local universe. In this contribution I review the role starbursts play in the…

Astrophysics · Physics 2009-10-31 Timothy M. Heckman

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…

Astrophysics · Physics 2015-11-11 Francois Schweizer

The strongest starbursts are observed towards galaxy nuclei, or circumnuclear regions. However in interacting galaxies, star formation is also triggered in overlap regions far from nuclei, in spiral arms and sometimes in tidal tails. What…

Astrophysics · Physics 2007-05-23 Francoise Combes

We argue that star formation in the disks of low-surface-brightness (LSB) galaxies shares a similar nature with that occurring in the far outer regions of normal-brightness spiral galaxies, such as those with the extended ultraviolet (XUV)…

Astrophysics of Galaxies · Physics 2025-08-12 A. V. Zasov , N. A. Zaitseva , A. S. Saburova

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…

Astrophysics of Galaxies · Physics 2022-09-21 Florent Renaud , Álvaro Segovia Otero , Oscar Agertz

Dusty galaxies with luminosities in excess of 10^11 solar luminosities have been detected out to redshifts of about unity by the Infrared Space Observatory (ISO), and to higher redshifts using millimetre(mm)- and submm-wave cameras on…

Astrophysics · Physics 2007-05-23 Andrew W. Blain

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…

Astrophysics of Galaxies · Physics 2023-09-19 Elia Cenci , Robert Feldmann , Jindra Gensior , Jorge Moreno , Luigi Bassini , Mauro Bernardini

This review presents a personal view of the role that starbursts play in the star formation history of the universe. It is mainly focused on the properties of nearby starburst galaxies selected for their strong UV and/or FIR emission. The…

Astrophysics · Physics 2007-10-26 Rosa M. Gonzalez Delgado

Mergers of massive gas-rich galaxies trigger violent starbursts that - over timescales of $> 100$ Myr and regions $> 10$ kpc - form massive and compact star clusters comparable in mass and radii to Galactic globular clusters. The star…

Astrophysics · Physics 2009-11-07 Uta Fritze-v. Alvensleben
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