The Evolution of a Computational Earth and Space Science Course
The evolution of a primordial binary population in a globular cluster
The evolution of a supernova remnant in a strongly magnetized interstellar medium
The evolution of a system of stars in an external environment
The evolution of black holes in an expanding universe
The evolution of cocoons surrounding light, extragalactic jets
The evolution of compact steep spectrum sources
The evolution of cooling flows - Self-similar cooling waves
The evolution of cooling flows. II - Galaxies and galaxy formation
The evolution of galaxies. IV - Highly flattened disks
The evolution of gravitational instabilities - Amplification by coupling of perturbation modes
The evolution of groups of galaxies in the Press-Schechter formalism
The evolution of He-burning stars - Horizontal and asymptotic branches in Galactic globulars
The evolution of helium stars in the mass range 2.0 to 4.0 solar masses - The evolutionary program
The evolution of horizontal-branch stars - Theoretical sequences
The evolution of inhomogeneities in expanding Newtonian cosmologies
The evolution of intermediate-mass stars through the H- and He-burning phases
The evolution of large-scale structure in a universe dominated by cold dark matter
The evolution of massive black-hole binaries in merging galaxies. I - Evolution of a binary in a spherical galaxy
The evolution of massive close binary systems with mass loss and overshooting. II - Case A of mass transfer in systems with high mass ratios