Results 71 to 80 of about 394,077 (286)

The M 101 group complex: new dwarf galaxy candidates and spatial structure [PDF]

open access: yes, 2017
Context. The fine details of the large-scale structure in the local Universe provide important empirical benchmarks for testing cosmological models of structure formation. Dwarf galaxies are key object for such studies. Aims.
O. Muller   +3 more
semanticscholar   +1 more source

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

Warp or lag? The ionized and neutral hydrogen gas in the edge-on dwarf galaxy UGC 1281 [PDF]

open access: yes, 2011
The properties of gas in the halos of galaxies constrain global models of the interstellar medium. Kinematical information is of particular interest since it is a clue to the origin of the gas. Until now mostly massive galaxies have been investigated for
Barbieri   +40 more
core   +3 more sources

APOGEE Chemical Abundances of the Sagittarius Dwarf Galaxy [PDF]

open access: yes, 2017
The Apache Point Observatory Galactic Evolution Experiment provides the opportunity of measuring elemental abundances for C, N, O, Na, Mg, Al, Si, P, K, Ca, V, Cr, Mn, Fe, Co, and Ni in vast numbers of stars.
S. Hasselquist   +28 more
semanticscholar   +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 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

UGC 7639: A Dwarf Galaxy in the Canes Venatici I Cloud

open access: yesAdvances in Astronomy, 2015
We want to get insight into the formation mechanism and the evolution of UGC 7639, a dwarf galaxy in the Canes Venatici I Cloud (CVnIC). We used archival multiwavelength data to constrain its global properties. Ultraviolet images show that UGC 7639 inner
L. M. Buson   +3 more
doaj   +1 more source

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

Discovery of Diffuse Dwarf Galaxy Candidates around M101 [PDF]

open access: yes, 2017
We have conducted a search of a 9 deg2 region of the Canada–France–Hawaii-Telescope Legacy Survey around the Milky Way analog M101 (D ∼ 7 Mpc), in order to look for previously unknown low-surface-brightness galaxies.
P. Bennet   +7 more
semanticscholar   +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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