Results 101 to 110 of about 52,385 (210)
This paper gives an overview of the attempts to determine the distribution of dark matter in low surface brightness disk and gas-rich dwarf galaxies, both through observations and computer simulations.
W. J. G. de Blok
doaj +1 more source
Comparing Galaxies and Lyman Alpha Absorbers at Low Redshift
A scenario is explored in which Lyman alpha absorbers at low redshift arise from lines of sight through extended galaxy disks, including those of dwarf and low surface brightness galaxies.
de Blok W. J. G. +11 more
core +1 more source
Galaxy clustering as a function of surface brightness [PDF]
Using diameters and magnitudes of galaxies listed in the Nilson catalog, the angular correlation properties of highand low-surface brightness galaxies are examined.
Davis, Marc, Djorgovski, S.
core
The radial profiles of the Hb, Mg, and Fe line-strength indices are presented for a sample of eight spiral galaxies with a low surface-brightness stellar disc and a bulge.
A. Pizzella +96 more
core +1 more source
The Intracluster Light of Abell 3667: Unveiling an Optical Bridge in LSST Precursor Data
Intracluster light (ICL), the diffuse glow of stars stripped from galaxies during a cluster’s formation, is an established tracer of a cluster’s dynamical history. The upcoming Vera C.
Anthony M. Englert +2 more
doaj +1 more source
LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies
We present an overview of the LBT Imaging of Galactic Halos and Tidal Structures survey, which currently includes 25 nearby galaxies that are on average ∼1 mag fainter than the Milky Way, and a catalog of 54 low central surface brightness (24 < μ _0, _g /
Dennis Zaritsky +14 more
doaj +1 more source
Oxygen abundances in low surface brightness disk galaxies
The oxygen abundances in the \HII regions of a sample of low surface brightness (LSB) disk galaxies are presented. In general, LSB galaxies are found to be metal poor ($Z < {1 \over 3} Z\solar$). Indeed, some LSB galaxies rival the lowest abundance extragalactic objects known. These low metallicities indicate that LSB galaxies evolve slowly, forming
openaire +2 more sources
We study massive disk galaxies (stellar mass > = 10 ^11 M _⊙ ) at z = 0 from IllustrisTNG simulation to detect galaxies that contain two exponential stellar disks—a central high surface brightness (HSB) disk surrounded by an extended low surface ...
Suchira Sarkar, Kanak Saha
doaj +1 more source
Searching for ultra-diffuse galaxies in the Dark Energy Survey using an object-detection algorithm
Ultra-diffuse galaxies (UDGs) are a class of galaxies characterized by an extremely low surface brightness and large effective radius. The significance of UDGs lies in their unique properties, such as their diverse dark-matter content, which collectively
Su Yiping +6 more
doaj +1 more source
Massive low surface brightness galaxies [PDF]
A multi-wavelength study of an extreme type of galaxy which will assist us in our attempts to understand the formation and evolution of galaxies was completed. In particular, a subset of low surface brightness (bar-mu(sub B) is approximately greater than
Knezek, Patricia M. +1 more
core +1 more source

