Results 31 to 40 of about 2,970 (256)

Anisotropies in the Distribution of Satellite Galaxies [PDF]

open access: yesThe Astrophysical Journal, 1997
15 pages, submitted to ...
Carlos S. Frenk   +3 more
openaire   +2 more sources

Self-interacting dark matter on small and large scales

open access: yesSciPost Physics Proceedings, 2023
In the self-interacting dark matter paradigm (hereafter SIDM), dark matter (DM) is assumed to have non-gravitational interactions with itself. SIDM has been constrained by observations of galaxy clusters. More recently, measurements of large DM densities
Camila A. Correa
doaj   +1 more source

Shock-induced Stripping of the Satellite Interstellar and Circumgalactic Medium in IllustrisTNG Clusters at Z ∼ 0

open access: yesThe Astrophysical Journal, 2023
Using the IllustrisTNG simulation, we study the interaction of large-scale shocks with the circumgalactic medium (CGM) and interstellar medium (ISM) of star-forming (SF) satellite galaxies in galaxy clusters.
Hao Li   +5 more
doaj   +1 more source

Shape Alignments of Satellite Galaxies [PDF]

open access: yesThe Astronomical Journal, 2002
4 pages, 2 figures, accepted for Aug 2002 Astronomical ...
Peder Norberg, Gary Bernstein
openaire   +2 more sources

More Satellites of Spiral Galaxies [PDF]

open access: yesThe Astrophysical Journal, 1997
We present a revised and expanded catalog of satellite galaxies of a set of isolated spiral galaxies similar in luminosity to the Milky Way. This sample of 115 satellites, 69 of which were discovered in our multifiber redshift survey, is used to further probe the results obtained from the original sample (Zaritsky et al. 1993).
Dennis Zaritsky   +3 more
openaire   +3 more sources

The colours of satellite galaxies in the Illustris simulation [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2014
Abstract Observationally, the fraction of blue satellite galaxies decreases steeply with host halo mass, and their radial distribution around central galaxies is significantly shallower in massive (M* ≥ 1011 M⊙) than in Milky Way-like systems.
Vicente Rodriguez-Gomez   +12 more
openaire   +7 more sources

A new spin on discs of satellite galaxies [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2015
We investigate the angular and kinematic distributions of satellite galaxies around a large sample of bright isolated primaries in the spectroscopic and photometric catalogues of the Sloan Digital Sky Survey (SDSS). We detect significant anisotropy in the spatial distribution of satellites.
Cautun, M.   +3 more
openaire   +5 more sources

DARK SATELLITES AND THE MORPHOLOGY OF DWARF GALAXIES [PDF]

open access: yesThe Astrophysical Journal, 2012
Submitted to ApJ Letters. 5 pages, 4 figures. A movie showing an encounter between a disky dwarf galaxy and a dark satellite can be found at http://www.astro.rug.nl/~ahelmi/dwarfs-morphologies ...
Amina Helmi   +7 more
openaire   +3 more sources

DWARF GALAXY CLUSTERING AND MISSING SATELLITES [PDF]

open access: yesThe Astrophysical Journal, 2009
At redshifts around 0.1 the CFHT Legacy Survey Deep fields contain some 6x10^4 galaxies spanning the mass range from 10^5 to 10^12 Msun. We measure the stellar mass dependence of the two point correlation using angular measurements to largely bypass the errors, approximately 0.02 in the median, of the photometric redshifts. Inverting the power-law fits
Carlberg, R. G.   +2 more
openaire   +4 more sources

The origin of lopsided satellite galaxy distribution in galaxy pairs [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
ABSTRACT It is well known that satellite galaxies are not isotropically distributed among their host galaxies as suggested by most interpretations of the Λ cold dark matter (ΛCDM) model. One type of anisotropy recently detected in the Sloan Digital Sky Survey (and seen when examining the distribution of satellites in the Local Group and ...
Chen Chris Gong   +13 more
openaire   +4 more sources

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