SiO line emission from C-type shock waves: interstellar jets and outflows

We study the production of SiO in the gas phase of molecular outflows, through the sputtering of Si-bearing material in refractory grain cores, which are taken to be olivine. We calculate also the rotational line spectrum of the SiO. The sputtering is driven by neutral particle impact on charged gra...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2008-05, Vol.482 (3), p.809-829
Hauptverfasser:	Gusdorf, A., Cabrit, S., Flower, D. R., Pineau des Forêts, G.
Format:	Artikel
Sprache:	eng
Schlagworte:	astrochemistry Astronomy Astrophysics atomic processes Earth, ocean, space Exact sciences and technology Galactic Astrophysics magnetohydrodynamics (MHD) molecular processes radiative transfer Sciences of the Universe shock waves
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