Elliptical (E) and spiral (S) galaxies follow tight, but different, scaling laws that link their stellar masses, radii, and characteristic velocities. Mass and velocity, for example, scale tightly in spirals with little dependence on galaxy radius (the ‘Tully-Fisher relation’; TFR). On the other hand, ellipticals appear to trace a 2D surface in size-mass-velocity space (the ‘Fundamental Plane’; FP). Over the years, a number of studies have attempted to understand these empirical relations, usually in terms of variations of the virial theorem for E galaxies and in terms of the scaling relations of dark matter halos for spirals. We use Lambda cold dark matter (ΛCDM) cosmological hydrodynamical simulations to show that the scaling relations of...
Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma...
By means of high-resolution N-body simulations in a LambdaCDM cosmology, we verify that scaling rela...
We study the evolution of the scaling relations between the maximum circular velocity, stellar mass ...
Elliptical (E) and spiral (S) galaxies follow tight, but different, scaling laws that link their ste...
Like early-type galaxies, nearby galaxy clusters also define fundamental plane, luminosity-radius, a...
Context. Two incorrect arguments against MOND in elliptical galaxies could be that the equivalent ci...
We investigate the structure of dark matter halos by means of the kinematics of a very large sample ...
International audienceDensity profiles (NFW and similar) of structures found in cosmological LambdaC...
Values of the M/L_B_ ratio in the inner regions of elliptical (E) galaxies are determined using ioni...
Values of the M/L(B) ratio in the inner regions of elliptical (E) galaxies are determined using ioni...
We present evidence that all galaxies, of any Hubble type and luminosity, bear the kinematical signa...
Dwarf elliptical galaxies are frequently excluded from bright galaxy samples because they do not fol...
Kinematic surveys of the dwarf spheroidal (dSph) satellites of the Milky Way are revealing tantalizi...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...
Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma...
Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma...
By means of high-resolution N-body simulations in a LambdaCDM cosmology, we verify that scaling rela...
We study the evolution of the scaling relations between the maximum circular velocity, stellar mass ...
Elliptical (E) and spiral (S) galaxies follow tight, but different, scaling laws that link their ste...
Like early-type galaxies, nearby galaxy clusters also define fundamental plane, luminosity-radius, a...
Context. Two incorrect arguments against MOND in elliptical galaxies could be that the equivalent ci...
We investigate the structure of dark matter halos by means of the kinematics of a very large sample ...
International audienceDensity profiles (NFW and similar) of structures found in cosmological LambdaC...
Values of the M/L_B_ ratio in the inner regions of elliptical (E) galaxies are determined using ioni...
Values of the M/L(B) ratio in the inner regions of elliptical (E) galaxies are determined using ioni...
We present evidence that all galaxies, of any Hubble type and luminosity, bear the kinematical signa...
Dwarf elliptical galaxies are frequently excluded from bright galaxy samples because they do not fol...
Kinematic surveys of the dwarf spheroidal (dSph) satellites of the Milky Way are revealing tantalizi...
We use a homogeneous sample of about 1100 optical and radio rotation curves (RCs); and relative surf...
Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma...
Axisymmetric, orbit-based dynamical models are used to derive dark matter scaling relations for Coma...
By means of high-resolution N-body simulations in a LambdaCDM cosmology, we verify that scaling rela...
We study the evolution of the scaling relations between the maximum circular velocity, stellar mass ...