Results 11 to 20 of about 151,190 (310)
Acknowledgment to Reviewers of Galaxies in 2020
Galaxies, 2021 Peer review is the driving force of journal development, and reviewers are gatekeepers who ensure that Galaxies maintains its standards for the high quality of its published papers [...]
Galaxies Editorial Office
doaj +2 more sources
Acknowledgement to Reviewers of Galaxies in 2016
Galaxies, 2017 The editors of Galaxies would like to express their sincere gratitude to the following reviewers for assessing manuscripts in 2016.[...]
Galaxies Editorial Office
doaj +2 more sources
Acknowledgement to Reviewers of Galaxies in 2014
Galaxies, 2015 The editors of Galaxies would like to express their sincere gratitude to the following reviewers for assessing manuscripts in 2014:[...]
Galaxies Editorial Office
doaj +2 more sources
An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic web. As galaxies are accreted they are affected by their local environment before they enter (pre-processing), and traverse the cluster potential.
Ulrike Kuchner +8 more
openaire +4 more sources
Acknowledgment to Reviewers of Galaxies in 2021
Galaxies, 2022 Rigorous peer-reviews are the basis of high-quality academic publishing [...]
Galaxies Editorial Office
doaj +1 more source
Acknowledgment to the Reviewers of Galaxies in 2022
Galaxies, 2023 High-quality academic publishing is built on rigorous peer review [...]
Galaxies Editorial Office
doaj +1 more source
Galaxy-galaxy(-galaxy) lensing as a sensitive probe of galaxy evolution [PDF]
Astronomy & Astrophysics, 2012 11 pages, 8 figures, accepted in A& ...
Saghiha, H. +3 more
openaire +3 more sources
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT We use cosmological simulations of isolated Milky Way (MW)-mass galaxies, as well as Local Group (LG) analogues, to define the ‘edge’ – a caustic manifested in a drop in density or radial velocity – of Galactic-sized haloes, both in dark matter and in stars.
Julio F Navarro +7 more
openaire +4 more sources
THE ORIENTATION OF GALAXIES IN GALAXY CLUSTERS [PDF]
The Astrophysical Journal, 2010 We present an analysis of the spatial orientations of galaxies in the 247 optically selected rich Abell clusters, having in the considered area at least 100 members. We investigated the relation between angles giving information about galaxy angular momenta and the number of members in each structure.
Godlowski, Wlodzimierz +3 more
openaire +2 more sources
Quasar-galaxy and galaxy-galaxy cross-correlations: model predictions with realistic galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2003 11 pages, 4 figures, matches version in ...
Jain, Bhuvnesh +2 more
openaire +2 more sources