Modelling the spectral energy distribution of galaxies. V. The dust and PAH emission SEDs of disk galaxies

Modelling the spectral energy distribution of galaxies: introducing the artificial neural network

Modelling the WMAP large-angle anomalies as an effect of a local density inhomogeneity

Modelling Time-varying Dark Energy with Constraints from Latest Observations

Models for the Clustering of Far-Infrared and Sub-millimetre selected Galaxies

Models of Accretion Disks

Models of evolution of gas and abundances in dwarf irregular galaxies

Models of high redshift luminosity functions and galactic outflows: The dependence on halo mass function

Models of Interacting Dark Energy

Models of Stephan's Quintet: Hydrodynamic Constraints on the Group's Evolution

Models of the Intergalactic Gas in Stephan's Quintet

Models of thin discs and spheroidal haloes with masses in a linear relationship: mass estimates for NGC4389 and UGC6969

Moderate Galaxy-Galaxy Lensing

Moderate Steepening of Galaxy Cluster Dark Matter Profiles by Baryonic Pinching

Modification of the 21-cm power spectrum by quasars during the epoch of reionisation

Modification of the halo mass function by kurtosis associated with primordial non-Gaussianity

Modified Chaplygin Gas and Constraints on its B parameter from CDM and UDME Cosmological models

Modified Chaplygin Gas as a Unified Dark Matter and Dark Energy Model and Cosmic Constraints

Modified Entropic Gravity and Cosmology

Modified f(G) gravity models with curvature-matter coupling