Results 41 to 50 of about 329,423 (212)

No assembly required: mergers are mostly irrelevant for the growth of low-mass dwarf galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
Author(s): Fitts, A; Boylan-Kolchin, M; Bullock, JS; Weisz, DR; El-Badry, K; Wheeler, C; Faucher-Giguere, CA; Quataert, E; Hopkins, PF; Keres, D; Wetzel, A; Hayward, CC | Abstract: © 2018 The Author(s).
Alex Fitts   +11 more
semanticscholar   +1 more source

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

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

Reignition of star formation in dwarf galaxies [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2018
The Local Group hosts a number of star-forming dwarf galaxies that show evidence of periods of little to no star formation. We use a suite of cosmological simulations to study how star formation is reignited in such galaxies.
A. Wright   +3 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   +6 more sources

Abundance ratios in dwarf elliptical galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2017
We determine abundance ratios of 37 dwarf ellipticals (dEs) in the nearby Virgo cluster. This sample is representative of the early-type population of galaxies in the absolute magnitude range -19.0 < Mr < -16.0. We analyze their absorption line-strength indices by means of index-index diagrams and scaling relations and use the stellar population ...
Jesús Falcón-Barroso   +21 more
openaire   +10 more sources

Giant halos in dwarf irregular galaxies vs. dwarf elliptical galaxies [PDF]

open access: yesProceedings of the International Astronomical Union, 2005
We present a discovery of a giant stellar halo in NGC 6822, a dwarf irregular galaxy in the Local Group. This halo is mostly made of old red giants, showing striking features: 1) it is several times larger than the main body of the galaxy seen in the optical images, and 2) it is elongated in the direction almost perpendicular to the HI disk of NGC 6822.
Narae Hwang, Myung Gyoon Lee
openaire   +4 more sources

The M dwarf problem in the Galaxy [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2012
To be published in Monthly Notices of the RAS by the Royal Astronomical Society and Blackwell Publishing.
Vincent M. Woolf, Andrew A. West
openaire   +4 more sources

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

On the dynamics of the Sagittarius dwarf galaxy [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1995
We use numerical simulations to test the feasibility of the suggestion by Ibata et al. (1994) that the excess population of stars which they discovered in the Sagittarius region may be the disrupted remains of a dwarf spheroidal galaxy. We find that a Fornax-like model for the pre-disruption system can indeed reproduce the data.
Hector Velazquez, Simon D. M. White
openaire   +2 more sources

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