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September 11, 2008Astronomy and Astrophysics180 citationsOpen Access

SiO line emission from interstellar jets and outflows: silicon-containing mantles and non-stationary shock waves

AGA. GusdorfGFG. Pineau des ForêtsSCS. Cabrit

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Abstract

Context. We study the production and emission of SiO and H in the gas phase of molecular outflows, extending previous work in which we considered steady-state C-type shock waves and assumed the silicon to be present only in the cores of silicate grains.

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Gusdorf et al. (2008) studied this question.

synapsesocial.com/papers/6a8358e5e60dbc776e30e85ehttps://doi.org/10.1051/0004-6361:200810443
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