Results 31 to 40 of about 24,234 (169)
Galaxy Groups at Intermediate Redshift [PDF]
Galaxy groups likely to be virialized are identified within the CNOC2 intermediate redshift galaxy survey using an iterative method. The number-velocity dispersion relation is in agreement with the low-mass extrapolation of the cluster normalized Press-Schechter function.
Carlberg, R. G. +7 more
openaire +3 more sources
A group of merging galaxies falling into Abell 2142
Galaxy clusters produce a very hostile environment for galaxies: their gas gets stripped by ram pressure, they undergo galaxy interactions, and their star formation is quenched.
Anitha Shaji Aashiya +5 more
doaj +1 more source
The shape of poor groups of galaxies [PDF]
7 pages, MNRAS accepted ...
Plionis, M. +2 more
openaire +2 more sources
Optical observations of M81 galaxy group in narrow band [SII] and Hα filters: Holmberg IX [PDF]
We present observations of the nearby tidal dwarf galaxy Holmberg IX in M81 galaxy group in narrow band [SII] and Hα filters, carried out in March and November 2008 with the 2m RCC telescope at NAO Rozhen, Bulgaria.
Arbutina B. +5 more
doaj +1 more source
The Fate of the Milky Way–Andromeda System: To Merge or Not?
It has long been predicted that the Milky Way (MW) will eventually merge with Andromeda (M31), a view reinforced by Hubble Space Telescope measurements indicating a small M31 transverse velocity. However, using updated Gaia-based proper motions (PMs) and
Hao Wu +4 more
doaj +1 more source
A Type Ia supernova (SN) at z = 1.78 was discovered in James Webb Space Telescope Near Infrared Camera imaging of the galaxy cluster PLCK G165.7+67.0 (G165; z = 0.35).
Brenda L. Frye +40 more
doaj +1 more source
Age Estimates for Galaxies in Groups [PDF]
AbstractWe discuss recent developments on the age and metallicity distribution for early type galaxies in different environments.
Forbes, Duncan, Terlevich, Alejandro I.
openaire +2 more sources
The M31–M33 Interaction: Impact on M31’s Center-of-mass Motion and Satellite Orbits
Inspired by recent studies of the interaction between the Milky Way and the Large Magellanic Cloud and its implications for the Milky Way’s global dynamical history, we investigate how the massive satellite galaxy M33 influences the position and velocity
Ekta Patel +2 more
doaj +1 more source
The PAndAS View of the Andromeda Satellite System. IV. Global Properties
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
Because groups are directly associated with halos, they allow for considerably simpler theoretical modeling than approaches based on individual galaxies.
Yingxiao Song +18 more
doaj +1 more source

