Tracing shocks in the BHR 71 protostellar outflow

Physics

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Stellar, Atca

Scientific paper

We propose to map the SiO 2-1 shocked emission along the length of the
redshifted BHR 71 protostellar molecular outflow, in order to resolve
the emission to compare directly with shocked H2 emission and to
determine the physical conditions within the high velocity emission.

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