Results 61 to 70 of about 399,477 (315)

Dwarf Spheroidal Galaxies [PDF]

open access: yesSymposium - International Astronomical Union, 1994
Dwarf Spheroidal (dSph) galaxies are the faintest baryonic systems recognized as galaxies. Understanding the structure and stellar populations of these systems is critical for the modelling of their formation and evolution, and by extension, for understanding the general problem of galaxy formation ...
openaire   +2 more sources

Magnetised winds in dwarf galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2010
20 pages, 12 figures.
Romain Teyssier   +3 more
openaire   +3 more sources

Dwarfs in Void Environments (DIVE): The Stellar Kinematics of Void Dwarf Galaxies Using the Keck Cosmic Web Imager

open access: yesThe Astrophysical Journal, 2023
Dwarf galaxies located in extremely underdense cosmic voids are excellent test beds for disentangling the effects of large-scale environments on galaxy formation and evolution. We present the first results of the Dwarfs in Void Environments Survey, which
Mithi A. C. de los Reyes   +5 more
doaj   +1 more source

Dwarf Galaxies in the Local Volume [PDF]

open access: yesAstrophysical Bulletin, 2018
AbstractThe Updated Nearby Galaxy Catalog (=UNGC) of 1047 Local Volume (=LV) galaxies, situated within a distance of 11 Mpc, contains 870 dwarfs, i.e. 5/6 of the sample. Almost 40% of them have accurate distances measured with Hubble Space Telescope. Most of the LV dwarfs have been observed in HI and Hα emission lines, as well in far-ultraviolet with ...
I. D. Karachentsev, Elena I. Kaisina
openaire   +4 more sources

THE NATURE OF RED DWARF GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2009
9 pages, 8 figures, Accepted for publication in ...
Wang, Y   +7 more
openaire   +5 more sources

Ultradiffuse galaxies: the high-spin tail of the abundant dwarf galaxy population [PDF]

open access: yes, 2016
Recent observations have revealed the existence of an abundant population of faint, low surface brightness (SB) galaxies, which appear to be numerous and ubiquitous in nearby galaxy clusters, including the Virgo, Coma and Fornax clusters.
N. Amorisco, Abraham Loeb
semanticscholar   +1 more source

Direct evidence of hierarchical assembly at low masses from isolated dwarf galaxy groups [PDF]

open access: yesNature Astronomy, 2017
The demographics of dwarf galaxy populations have long been in tension with predictions from the Λ cold dark matter (ΛCDM) paradigm1–4. If primordial density fluctuations were scale-free as predicted, dwarf galaxies should themselves host dark-matter ...
S. Stierwalt   +7 more
semanticscholar   +1 more source

From tidal dwarf galaxies to satellite galaxies [PDF]

open access: yesAstronomy & Astrophysics, 2006
Accepted for publication in A&A. Shortened abstract below, full version in the paper.
Bournaud, Frédéric, Duc, Pierre-Alain
openaire   +5 more sources

A Comparison of Outflow Properties in AGN Dwarfs versus Star-forming Dwarfs

open access: yesThe Astrophysical Journal, 2023
Feedback likely plays a crucial role in resolving discrepancies between observations and theoretical predictions of dwarf galaxy properties. Stellar feedback was once believed to be sufficient to explain these discrepancies, but it has thus far failed to
Archana Aravindan   +7 more
doaj   +1 more source

Metallic Winds in Dwarf Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2017
Abstract We present results from models of galactic winds driven by energy injected from nuclear (at the galactic center) and non-nuclear starbursts. The total energy of the starburst is provided by very massive young stellar clusters, which can push the galactic interstellar medium and produce an important outflow. Such outflow can be a
F. Robles-Valdez   +3 more
openaire   +3 more sources

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