Hypersonic Molecular Shocks in Star Forming Regions

Details Hypersonic Molecular Shocks in Star Forming Regions Hypersonic Molecular Shocks in Star Forming Regions

2006-09-08

arxiv.org/abs/astro-ph/0609234v1

Astronomy and Astrophysics

Astrophysics

To be published as a chapter in 'Diffuse Matter from Star Forming Regions to Active Galaxies' - A volume Honouring John Dyson.

Scientific paper

Much emission from star forming regions is from shock-excited gas. Shocks in
molecular clouds are still not fully understood, as magnetic fields, dust and
chemistry all play significant roles. I review the history, physics and current
work in understanding these shocks, and in their possible use as diagnostics of
local conditions.

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