Kinematics and dynamics of diffuse astrophysical media; Manchester Conference, 8th, Manchester, UK, Mar. 22-26, 1993

Details Kinematics and dynamics of diffuse astrophysical media; Manchester Conference, 8th, Manchester, UK, Mar. 22-26, 1993 Kinematics and dynamics of diffuse astrophysical media; Manchester Conference, 8th, Manchester, UK, Mar. 22-26, 1993

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216.....d&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, 401 p.

Astronomy and Astrophysics

Astrophysics

Astronomical Models, Astronomy, Astrophysics, Galactic Evolution, Gas Dynamics, Gas Flow, Interstellar Gas, Interstellar Matter, Kinematics, Magnetohydrodynamic Flow, Molecular Clouds, Plasma Jets, Stellar Envelopes, Stellar Evolution, Stellar Winds, Astronomical Spectroscopy, Galactic Halos, Galactic Structure, Interplanetary Dust, Interstellar Chemistry, Magnetohydrodynamics, Plasma Interactions, Radio Sources (Astronomy), Relativistic Plasmas, Shock Wave Interaction, Shock Waves, Star Formation, Stellar

Scientific paper

The area of diffuse astrophysical media is enormous and ranges over circumstellar to extragalactic scales. The physical conditions vary from cool dusty gases to collections of relativistic particles. Flows in such media are set up by energy and momentum injection from winds, jets, and explosions. The study of these phenomena involves physics, chemistry, and hydrodynamics. One of the most important aspects of this study is the ever increasing overlap between theory and observation. Indeed, it can be argued that the only way to really understand these complex flows, which can never be duplicated under terrestrial conditions, is to encourage this overlap, and this was one major aim of this conference. For individual titles, see A95-64759 through A95-64824.

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