Theory of interstellar shocks ADS Classic is now deprecated. It will be completely retired in
October 2019. This page will automatically redirect to the new ADS interface at that point …

Recent progress in the detection of H2 in the interstellar medium is reviewed. The hydrogen
molecule is discussed in terms of properties, and collisional excitation and dissociation …

The paper analyzes the structure of fast shocks incident upon interstellar gas of ambient
density from 10 to the 7th per cu cm, while focusing on the problems of formation and …

Nondissociative, magnetohydrodynamic, C-type shock waves are expected to be a
prodigious source of far-infrared water emissions in dense interstellar regions. We have …

When I started working on my PhD project on X-ray spectroscopy of supernova remnants in
1995, one of the things that I missed was a good textbook covering the various aspects of …

We have used a coupled time-dependent chemical and dynamical model to investigate the
lifetime of the chemical legacy in the wake of C-type shocks. We concentrate this study on …

Ambipolar diffusion in self-gravitating isothermal layers ADS Classic is now deprecated. It will
be completely retired in October 2019. This page will automatically redirect to the new ADS …

Context. Large-scale motions in galaxies (supernovae explosions, galaxy collisions, galactic
shear etc.) generate turbulence, which allows a fraction of the available kinetic energy to …

In the interstellar medium-the space between the stars in galaxies-new stars are born from
material that is replenished by the debris ejected by stars when they die. This book is a …

We have computed two-fluid MHD models of shocks propagating in molecular clouds of
density 104≤ n H≤ 106 cm–3, with speeds of 5≤ υs≤ 40 km s–1. Attention has been paid …