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Mineralogy of an OH/IR superwind
DOI: 10.1088/1742-6596/728/2/022004 Bibcode: 2016JPhCS.728b2004L

Lombaert, R.; de Vries, B. L.; Hillen, M.

The mineralogy of the dense, dusty superwind of OH/IR stars can provide important constraints for understanding the dust formation process as well as the acceleration of the wind. We aim to model the ISO-SWS spectrum of the OH/IR star OH 30.1-0.7 in detail by reproducing the slope of the spectral energy distribution in the continuum regions betwee…

2016 Journal of Physics Conference Series
ISO 0