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Dwarf galaxies play an important role in our understanding of galaxy formation and evolution, and starbursts are believed to strongly affect their structure and evolution. Here we present a study of 12 of the nearest dwarf galaxies thought…

天体物理学 · 物理学 2009-10-31 Amanda T. Marlowe , Gerhardt R. Meurer , Timothy M. Heckman

The aim of this paper is to cast light on the formation and evolution of elliptical galaxies by means of N-body/hydro-dynamical simulations that include star formation, feed-back and chemical evolution. Particular attention is paid to the…

天体物理学 · 物理学 2009-11-06 G. Carraro , C. Chiosi , L. Girardi , C. Lia

Properties of nearby dwarf galaxies are briefly discussed. Dwarf galaxies vary widely in their star formation histories, the ages of their subpopulations, and in their enrichment history. Furthermore, many dwarf galaxies show evidence for…

天体物理学 · 物理学 2009-10-31 Eva K. Grebel

An unresolved question in galaxy evolution is whether the star formation histories of low mass systems are preferentially dominated by starbursts or modes that are more quiescent and continuous. Here, we quantify the prevalence of global…

天体物理学 · 物理学 2010-03-19 Janice C. Lee , Robert C. Kennicutt , José G. Funes S. J. , Shoko Sakai , Sanae Akiyama

Star forming dwarf galaxies (SFDGs) have a high gas content and low metallicities, reminiscent of the basic entities in hierarchical galaxy formation scenarios. In the young universe they probably also played a major role in the cosmic…

星系天体物理 · 物理学 2015-05-28 Nils Bergvall

Dwarf galaxies in the Local Group appear to be stripped of their gas within 270 kpc of the host galaxy. Color-magnitude diagrams of these dwarfs, however, show clear evidence of episodic star formation (\Delta{}t ~ a few Gyr) over cosmic…

宇宙学与河外天体物理 · 物理学 2015-05-30 Matthew Nichols , Doug Lin , Joss Bland-Hawthorn

The results of UBV and H alpha imaging of a large sample of isolated dwarf irregular galaxies are interpreted in the context of composite stellar population models. The observed optical colors are best fit by composite stellar populations…

天体物理学 · 物理学 2009-08-17 L. van Zee

I review the evolutionary status of the field populations of starbursting dwarf galaxies and low surface brightness spirals. Particular attention is paid to the long standing problem of the progenitors for star burst galaxies, which may be…

天体物理学 · 物理学 2007-05-23 Stacy S. McGaugh

The starburst phenomenon can shape the evolution of the host galaxy and the surrounding intergalactic medium. The extent of the evolutionary impact is partly determined by the duration of the starburst, which has a direct correlation with…

We examine the star formation history and stellar feedback effects of dwarf galaxies under the influence of extragalactic ultraviolet radiation. We consider the dynamical evolution of gas in dwarf galaxies using a one-dimensional,…

天体物理学 · 物理学 2009-11-10 Shawfeng Dong , D. N. C. Lin , S. D. Murray

The duration of a starburst is a fundamental parameter affecting the evolution of galaxies yet, to date, observational constraints on the durations of starbursts are not well established. Here we study the recent star formation histories…

Dwarf galaxy star formation histories are theoretically expected to be bursty, potentially leaving distinct imprints on their chemical evolution. We propose that episodic starbursts with quiescent periods longer than $\sim$100 Myr should…

星系天体物理 · 物理学 2025-01-20 Yuan-Sen Ting , Alexander P. Ji

It has been proposed that mergers induce starbursts and lead to important morphological changes in galaxies. Most studies so far have focused on large galaxies, but dwarfs might also experience such events, since the halo mass function is…

星系天体物理 · 物理学 2016-02-17 Tjitske K. Starkenburg , Amina Helmi , Laura V. Sales

Growing evidence has been accumulated for that some gas-rich dwarf galaxies are formed from material liberated by galaxy collisions and/or mergers. Also, gas-poor dwarf elliptical galaxies are often found in the central regions of clusters…

天体物理学 · 物理学 2009-10-31 T. Okazaki , Y. Taniguchi

The optical/near-IR stellar continuum carries unique information about the stellar population in a galaxy, its mass function and star-formation history. Star-forming regions display rich emission-line spectra from which we can derive the…

天体物理学 · 物理学 2015-11-11 Nils Bergvall , Thomas Marquart , Göran Östlin , Erik Zackrisson

The properties and star formation processes in the far-outer disks of nearby spiral and dwarf irregular galaxies are reviewed. The origin and structure of the generally exponential profiles in stellar disks is considered to result from…

星系天体物理 · 物理学 2017-08-02 Bruce G. Elmegreen , Deidre A. Hunter

Galaxy counts from bright ultraviolet (UV) and deep optical spectroscopic surveys have revealed an unexpectedly large number of very blue galaxies. The colors and luminosities of these objects indicate that they are dwarf galaxies…

天体物理学 · 物理学 2007-05-23 Michel Fioc , Brigitte Rocca-Volmerange

Early-type dwarf galaxies are the most common type of galaxies observed in the Universe. The origin of this kind of systems is still not well understood. The aim of this paper is to investigate whether the different locations of dwarf…

天体物理学 · 物理学 2009-11-13 J. A. L. Aguerri , C. Gonzalez-Garcia

Strong bursts of star formation in galaxies may be triggered either by internal or external mechanisms. We study the distribution and kinematics of the HI gas in the outer regions of 18 nearby starburst dwarf galaxies, that have accurate…

星系天体物理 · 物理学 2015-06-22 Federico Lelli , Marc Verheijen , Filippo Fraternali

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…

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