The alignment and shape of dark matter, stellar, and hot gas distributions in the EAGLE and cosmo-OWLS simulations (2015)
Attributed to:
The Virgo consortium for cosmological supercomputer simulations
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stv1690
Publication URI: http://dx.doi.org/10.1093/mnras/stv1690
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1