Shock Models Revisited

Details Shock Models Revisited Shock Models Revisited

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005iaus..231..135w&link_type=abstract

Astrochemistry: Recent Successes and Current Challenges, Proceedings of the 231st Symposium of the International Astronomical Un

Astronomy and Astrophysics

Astronomy

2

Scientific paper

We review progress in the area of the modelling of shocks in molecular clouds. In particular, we consider what has been learnt about shock structure evolution in situations where the steady-state assumption is no longer valid. We discuss the interpretation of the observed water abundance from SWAS, Odin, and ISO. We also consider the erosion of grains in shocks as well as the effect of the presence of grains on shock structure.

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