Cloud collisions and depletion of CNO-elements

Details Cloud collisions and depletion of CNO-elements Cloud collisions and depletion of CNO-elements

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45..103y&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Physics

Astronomical Models, Cloud Physics, Collision Parameters, Gas Dynamics, Stellar Evolution, Dynamic Models, Gas Density, Gas Pressure, Hydrogen Clouds, Interstellar Gas, Shock Waves

Scientific paper

A hydrodynamic model is used to calculate the evolution of two identical interstellar clouds colliding supersonically. The evolution of the clouds is divided into two phases: (1) the phase of rapid compression, during which the density of the cloud material is sharply reduced due to the passage of two shock waves through the gas, and (2) the oscillatory phase, which involves the oscillation of the compressed gas about the equilibrium density and pressure configuration on a dynamic time scale. The partial differential equations for the cloud-cloud collision are solved numerically.

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