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Related papers: BreakBRD Galaxies: Evolutionary Clues Through an A…

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Observed breakBRD ("break bulges in red disks") galaxies are a nearby sample of face-on disk galaxies with particularly centrally-concentrated star formation: they have red disks but recent star formation in their centers as measured by the…

Astrophysics of Galaxies · Physics 2023-08-09 Stephanie Tonnesen , Daniel DeFelippis , Sarah Tuttle

The observed breakBRD ("break bulges in red disks") galaxies are a nearby sample of face-on disk galaxies with particularly centrally concentrated star formation: they have red disks but recent star formation in their centers as measured by…

Astrophysics of Galaxies · Physics 2025-06-26 Claire Kopenhafer , Tjitske K. Starkenburg , Stephanie Tonnesen , Sarah Tuttle

We introduce a collection of primarily centrally star-forming galaxies that are selected by disk color to have truncated disk star formation. We show that common explanations for centrally-concentrated star formation -- low stellar mass,…

Astrophysics of Galaxies · Physics 2020-02-12 Sarah E. Tuttle , Stephanie Tonnesen

Studying the gas content of post-starburst (PSB) galaxies can provide valuable clues regarding the process of fast quenching. Although previous works have studied the molecular gas content of PSBs, only a handful of HI measurements exist.…

We have obtained new HI observations with the 100m Green Bank Telescope (GBT) for a sample of 29 extremely metal-deficient star-forming Blue Compact Dwarf (BCD) galaxies, selected from the Sloan Digital Sky Survey spectral data base to be…

Astrophysics of Galaxies · Physics 2023-05-03 T. X. Thuan , K. M. Goehring , J. E. Hibbard , Y. I. Izotov , L. K. Hunt

Until recently, dust emission has been detected in very few host galaxies of gamma-ray bursts (GRBHs). With Herschel, we have now observed 17 GRBHs up to redshift z~3 and detected seven of them at infrared (IR) wavelengths. This relatively…

We have collected an heterogeneous sample of galaxies at redshifts 0.001<z<3.35 with the aim of exploring the evolution of the physical parameters and of the element abundances calculated by modelling the observed spectra. The evolution…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-22 M. Contini

Recent work has identified a population of low-redshift E/S0 galaxies that lie on the blue sequence in color vs. stellar mass parameter space, where spiral galaxies typically reside. While high-mass blue-sequence E/S0s often resemble young…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 L. H. Wei , S. J. Kannappan , S. N. Vogel , A. J. Baker

We present Arecibo 21 cm spectroscopy, Keck HIRES Hb spectroscopy, and WIYN R-band images of 11 nearby blue compact galaxies selected to be similar to blue compact star-forming galaxies at intermediate redshifts (0.1<z<1). We detect HI in…

Astrophysics · Physics 2009-11-06 D. J. Pisano , Henry A. Kobulnicky , Rafael Guzman , Jesus Gallego , Matthew A. Bershady , ;

We present a demographic analysis of integrated star formation and gas properties for a sample of galaxies representative of the overall population at z~0. This research was undertaken in order to characterise the nature of star formation…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 M. S. Bothwell , R. C. Kennicutt , J. C. Lee

This is the fourth paper in a series studying star formation rates, stellar components, metallicities, and star formation histories of a blue compact galaxy (BCG) sample. Using Ha, [OII]3727, IR, radio (1.4GHz) luminosities and neutral…

Astrophysics · Physics 2009-11-10 Xu Kong

Star-forming galaxies populate a main sequence (MS), a well-defined relation between stellar mass (M*) and star-formation rate (SFR). Starburst (SB) galaxies lie significantly above the relation whereas quenched galaxies lie below the…

We investigate the evolutionary pathways of green valley (GV) galaxies drawn from the SDSS-IV/MaNGA survey. The GV sample is divided into fast- and slow-rotating galaxies based on stellar spin, and their stellar and gas-phase metallicities…

Astrophysics of Galaxies · Physics 2026-04-29 Shuang Zhou , Angela Iovino , Marcella Longhetti , Francesco La Barbera , Luca Costantin

We calculate the physical conditions and the N/H and O/H relative abundances for a sample of long GRB (LGRB) host galaxies in the redshift range 1<z<2.1 by modelling recently observed line and continuum spectra. The results are consistent…

Astrophysics of Galaxies · Physics 2020-06-02 Marcella Contini

We aim to unravel the interplay between bars, star formation (SF), and active galactic nuclei (AGNs) in barred galaxies. To this end, we utilize the SDSS DR12 to select a sample of nearby (0.02 < z < 0.06) disk galaxies that are suitable…

Astrophysics of Galaxies · Physics 2023-06-07 Woong-Bae G. Zee , Sanjaya Paudel , Jun-Sung Moon , Suk-Jin Yoon

We study the atomic Hydrogen (HI) content of galaxies in the core of the Shapley Supercluster (SSC) at <z> ~ 0.048, using observations from the MeerKAT Galaxy Cluster Legacy Survey and optical data from the Shapley Supercluster Survey…

Astrophysics of Galaxies · Physics 2026-04-10 L. Gwebushe , T. Venturi , P. Merluzzi , G. Busarello , V. Casasola , O. Smirnov , M. Ramatsoku , J. Dawson

The hosts of long duration gamma-ray bursts are predominantly starburst galaxies at subsolar metallicity. At redshifts z<1, this implies that most of them are low-mass galaxies similar to the populations of blue compact dwarfs and dwarf…

(Abridged) We investigate the properties of galaxies between the blue and the red sequence (i.e., the transition region) by combining UV and NIR imaging to HI line observations for a volume-limited sample of nearby galaxies. We confirm the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 L. Cortese , T. M. Hughes

We investigate the dynamics of starbursting dwarf galaxies, using both new and archival HI observations. We consider 18 nearby galaxies that have been resolved into single stars by HST observations, providing their star formation history…

Astrophysics of Galaxies · Physics 2014-06-23 Federico Lelli , Marc Verheijen , Filippo Fraternali

For a rotating galaxy, the inner circular-velocity gradient d_{R}V(0) provides a direct estimate of the central dynamical mass density, including gas, stars, and dark matter. We consider 60 low-mass galaxies with high-quality HI and/or…

Astrophysics of Galaxies · Physics 2014-03-05 Federico Lelli , Filippo Fraternali , Marc Verheijen
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