A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
Elena Arjona-Gálvez(Universidad de La Laguna), Alexander Knebe(Universidad Autónoma de Madrid), Claudio Dalla Vecchia, Noam I. Libeskind(Leibniz Institute for Astrophysics Potsdam), Robert J. J. Grand(Heidelberg University), José A. Benavides(University of California, Riverside), Andrea V. Macciò(New York University Abu Dhabi), Salvador Cardona–Barrero(Universidad de La Laguna), Arianna Di Cintio
Cited by 7
Related Papers
The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
|Monthly Notices of the Royal Astronomical Society|2017|556
Tracing the cosmic web
|Monthly Notices of the Royal Astronomical Society|2017|342
A kinematic classification of the cosmic web
|Monthly Notices of the Royal Astronomical Society|2012|189
The Orbital Poles of Milky Way Satellite Galaxies: A Rotationally Supported Disk of Satellites
|The Astrophysical Journal|2008|166
TWO PLANES OF SATELLITES IN THE CENTAURUS A GROUP
|The Astrophysical Journal Letters|2015|148