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相关论文: Starbursts, Dark Matter and Dwarf Galaxy Evolution

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We have explored the role environmental factors play in determining characteristics of young stellar objects in nearby dwarf irregular and Blue Compact Dwarf galaxies. Star clusters are characterized by concentrations, masses, and formation…

In this paper, the evolution of galaxies is by the incompatibility between dark matter and baryonic matter. Due to the structural difference, baryonic matter and dark matter are incompatible to each other as oil droplet and water in…

高能物理 - 理论 · 物理学 2011-02-11 Ding-Yu Chung

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…

天体物理学 · 物理学 2007-05-23 Andrew W. Blain

The concordance cosmological model based on cold dark matter makes definitive predictions for the growth of galaxies in the Universe, which are being actively studied using numerical simulations. These predictions appear to contradict the…

天体物理学 · 物理学 2015-06-24 Oleg Y. Gnedin

In the standard cosmological model, dark matter drives the structure formation and constructs potential wells within which galaxies may form. The baryon fraction in dark halos can reach the universal value (15.7%) in massive clusters and…

星系天体物理 · 物理学 2019-12-05 Qi Guo , Huijie Hu , Zheng Zheng , Shihong Liao , Wei Du , Shude Mao , Linhua Jiang , Jing Wang , Yingjie Peng , Liang Gao , Jie Wang , Hong Wu

The formation mechanism of high-concentration dwarf galaxies is still a mystery. We perform a comparative study of the intrinsic shape of nearby low-mass galaxies with different stellar concentration. The intrinsic shape is parameterized by…

星系天体物理 · 物理学 2023-09-12 Lijun Chen , Hong-Xin Zhang , Zesen Lin , Guangwen Chen , Bojun Tao , Zhixiong Liang , Zheyu Lin , Xu Kong

The ubiquity of star-forming dwarf galaxies (SFDG) in the local Universe allows us to trace their evolution in all type of environments, from voids to rich clusters. SFDGs in low-density regions are still assembling their mass, they often…

星系天体物理 · 物理学 2020-01-08 M. Grossi

In this second paper of a series, we explore the B-V, U-B, and FUV-NUV radial color trends from a multi-wavelength sample of 141 dwarf disk galaxies. Like spirals, dwarf galaxies have three types of radial surface brightness profiles: (I)…

星系天体物理 · 物理学 2016-06-06 Kimberly A. Herrmann , Deidre A. Hunter , Bruce G. Elmegreen

Dwarf galaxies (DGs) are extremely challenging objects in extragalactic astrophysics. They are expected to originate as the first units in Cold Dark-Matter cosmology. They are the galaxy type most sensitive to environmental influences and…

宇宙学与河外天体物理 · 物理学 2015-06-05 Gerhard Hensler

Low-mass galaxies radio observations show in many cases surprisingly high levels of magnetic field. The mass and kinematics of such objects do not favour the development of effective large-scale dynamo action. We attempted to check if the…

星系天体物理 · 物理学 2018-03-14 Hubert Siejkowski , Marian Soida , Krzysztof T. Chyzy

Optical observations of Blue Compact Dwarf galaxies (BCDs) show they typically have high specific star formation rates and low metallicites. A subset of these galaxies (those with the lowest gas phase metallicities) display cometary optical…

星系天体物理 · 物理学 2025-01-06 Tom C. Scott , Elias Brinks , Chandreyee Sengupta , Patricio Lagos

In this paper we present some results concerning the effects of two instantaneous starbursts, separated by a quiescent period, on the dynamical and chemical evolution of blue compact dwarf galaxies. In particular, we compare the model…

天体物理学 · 物理学 2009-11-07 S. Recchi , F. Matteucci , A. D'Ercole , M. Tosi

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

We present deep $BVI$ observations of the dwarf irregular galaxy UKS1927-177 in Sagittarius. Statistically cleaned $V$, $(B-I)$ CMDs clearly display the key evolutionary features in this galaxy. Previously detected C stars are located in…

天体物理学 · 物理学 2009-11-07 Y. Momany , E. V. Held , I. Saviane , L. Rizzi

In this paper, we report our studies on the gaseous and chemical properties of a relatively large sample (53 members) of blue compact dwarf galaxies (BCDs). The results of correlations among the oxygen abundance, stellar mass, gas mass,…

宇宙学与河外天体物理 · 物理学 2013-01-28 Yinghe Zhao , Yu Gao , Qiusheng Gu

We present the largest sample of brown dwarf (BD) protoplanetary disk spectral energy distributions modeled to date. We compile 49 objects with ALMA observations from four star-forming regions: $\rho$ Ophiuchus, Taurus, Lupus, and Upper…

太阳与恒星天体物理 · 物理学 2021-11-24 Anneliese M. Rilinger , Catherine C. Espaillat

The extent to which star formation varies in galaxies with low masses, low metallicities, and high star formation rate surface densities is not well-constrained. To gain insight into star formation under these physical conditions, this…

星系天体物理 · 物理学 2015-06-18 Amanda A. Kepley , Amy E. Reines , Kelsey E. Johnson , Lisa May Walker

In this review I summarise recent advances in our understanding of the importance of starburst events to the evolutionary histories of nearby galaxies. Ongoing bursts are easily diagnosed in emission-line surveys, but assessing the timing…

星系天体物理 · 物理学 2015-05-14 Andrew A. Cole

Moderately luminous starbursts in the nearby universe often occur in disk galaxies that are at most subject to mild external perturbations. An investigation of this type of galaxy leads to a better understanding of starburst triggering…

天体物理学 · 物理学 2007-05-23 John S. Gallagher , Christopher J. Conselice , Lynn D. Matthews , Nicole L. Homeier

We identify and characterize compact dwarf starburst (CDS) galaxies in the RESOLVE survey, a volume-limited census of galaxies in the local universe, to probe whether this population contains any residual ``blue nuggets,'' a class of…