Results 51 to 60 of about 527,839 (302)

Dwarfs from the Dark (Energy Survey): a machine learning approach to classify dwarf galaxies from multi-band images

open access: yesThe Open Journal of Astrophysics, 2021
Countless low-surface brightness objects - including spiral galaxies, dwarf galaxies, and noise patterns - have been detected in recent large surveys.
Oliver Müller, Eva Schnider
doaj   +1 more source

Radio jets from AGNs in dwarf galaxies in the COSMOS survey: mechanical feedback out to redshift ∼3.4 [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
Dwarf galaxies are thought to host the remnants of the early Universe seed black holes (BHs) and to be dominated by supernova feedback. However, recent studies suggest that BH feedback could also strongly impact their growth. We report the discovery of
M. Mezcua, H. Suh, F. Civano
semanticscholar   +1 more source

Globular Clusters and the Halos of Dwarf Galaxies

open access: yesGalaxies, 2017
Many dwarf galaxies have disproportionately rich globular cluster (GC) systems for their luminosities. Moreover, the GCs tend to be preferentially associated with the most metal-poor stellar populations in their parent galaxies, making them attractive ...
Søren S. Larsen
doaj   +1 more source

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

NIHAO XV: the environmental impact of the host galaxy on galactic satellite and field dwarf galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
We study the impact of the host on dwarf galaxy properties using four new Milky Way-like, ultra high-resolution simulations, ($N_{\rm part} >10^7$) from the NIHAO project. We split our sample in satellite ($R 2.5 R_{\rm 200}$) galaxies.
T. Buck   +4 more
semanticscholar   +1 more source

The PAndAS View of the Andromeda Satellite System. IV. Global Properties

open access: yesThe Astrophysical Journal, 2023
We build a statistical framework to infer the global properties of the satellite system of the Andromeda galaxy (M31) from the properties of individual dwarf galaxies located in the Pan-Andromeda Archaelogical Survey (PAndAS) and the previously ...
Amandine Doliva-Dolinsky   +10 more
doaj   +1 more source

Multimessenger Signatures of Massive Black Holes in Dwarf Galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
Recent discoveries of massive black holes (MBHs) in dwarf galaxies suggest that they may have a more common presence than once thought. Systematic searches are revealing more candidates, but this process could be accelerated by predictions from ...
J. Bellovary   +6 more
semanticscholar   +1 more source

THE METALLICITY OF VOID DWARF GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2014
The current Lambda CDM cosmological model predicts that galaxy evolution proceeds more slowly in lower density environments, suggesting that voids are a prime location to search for relatively pristine galaxies that are representative of the building blocks of early massive galaxies.
K. Kreckel   +4 more
openaire   +4 more sources

Substructure in Dwarf Galaxies [PDF]

open access: yesPublications of the Astronomical Society of Australia, 2004
AbstractRecent years have seen a series of large-scale photometric surveys with the aim of detecting substructure in nearby dwarf galaxies. Some of these objects display a varying distribution of each stellar population, reflecting their star formation histories.
openaire   +4 more sources

Pushing back the limits: detailed properties of dwarf galaxies in a ΛCDM universe [PDF]

open access: yesAstronomy & Astrophysics, 2018
We present the results of a set of high-resolution chemo-dynamical simulations of dwarf galaxies in a ΛCDM cosmology. Out of an original (3.4 Mpc/h)3 cosmological box, a sample of 27 systems are re-simulated from z = 70 to z = 0 using a zoom-in technique.
Y. Revaz, P. Jablonka
semanticscholar   +1 more source

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