none17noneEvrard A.E.; Bialek J.; Busha M.; White M.; Habib S.; Heitmann K.; Warren M.; Rasia E. ;Tormen G.; Moscardini L.; Power C.; Jenkins A.R.; Gao L.; Frenk C.S.; Springel V.; White S.D.M.; Diemand J.Evrard A.E.; Bialek J.; Busha M.; White M.; Habib S.; Heitmann K.; Warren M.; Rasia E. ;Tormen G.; Moscardini L.; Power C.; Jenkins A.R.; Gao L.; Frenk C.S.; Springel V.; White S.D.M.; Diemand J
Like early-type galaxies, nearby galaxy clusters also define fundamental plane, luminosity-radius, a...
To describe the density profile of dark matter halos of clusters of galaxies, we compare the approac...
We explore the dependence of the central logarithmic slope of dark matter halo density profiles 	...
We present a precise estimate of the bulk virial scaling relation of halos formed via hierarchical ...
We present a precise estimate of the bulk virial scaling relation of halos formed via hierarchical c...
We explore the effects of dark matter and dark energy on the dynamical scaling properties of galaxy ...
We use a set of large cosmological N-body simulations to study the internal structure of dark matter...
Virial mass is used as an estimator for the mass of a dark matter halo. However, the commonly used c...
International audienceThe halo shape plays a central role in determining important observational pro...
We investigate the structure of dark matter halos by means of the kinematics of a very large sample ...
We measure the clustering of dark matter halos in a large set of collisionless cosmological simulati...
We use N-body simulations to investigate the structure of dark halos in the standard Cold Dark Matte...
High-resolution LCDM cosmological N-body simulations are used to study the properties of galaxy-size...
We use the Chandra X-ray Observatory to study the dark matter halos of 34 massive, dynamically relax...
We investigated the structure of the dark matter halo formed in the cold dark matter scenarios by N...
Like early-type galaxies, nearby galaxy clusters also define fundamental plane, luminosity-radius, a...
To describe the density profile of dark matter halos of clusters of galaxies, we compare the approac...
We explore the dependence of the central logarithmic slope of dark matter halo density profiles 	...
We present a precise estimate of the bulk virial scaling relation of halos formed via hierarchical ...
We present a precise estimate of the bulk virial scaling relation of halos formed via hierarchical c...
We explore the effects of dark matter and dark energy on the dynamical scaling properties of galaxy ...
We use a set of large cosmological N-body simulations to study the internal structure of dark matter...
Virial mass is used as an estimator for the mass of a dark matter halo. However, the commonly used c...
International audienceThe halo shape plays a central role in determining important observational pro...
We investigate the structure of dark matter halos by means of the kinematics of a very large sample ...
We measure the clustering of dark matter halos in a large set of collisionless cosmological simulati...
We use N-body simulations to investigate the structure of dark halos in the standard Cold Dark Matte...
High-resolution LCDM cosmological N-body simulations are used to study the properties of galaxy-size...
We use the Chandra X-ray Observatory to study the dark matter halos of 34 massive, dynamically relax...
We investigated the structure of the dark matter halo formed in the cold dark matter scenarios by N...
Like early-type galaxies, nearby galaxy clusters also define fundamental plane, luminosity-radius, a...
To describe the density profile of dark matter halos of clusters of galaxies, we compare the approac...
We explore the dependence of the central logarithmic slope of dark matter halo density profiles 	...