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Article contents
Is there a signature of ice in the IRAS LRS spectra of some Mira variables?
Published online by Cambridge University Press: 04 August 2017
Extract
Some M Miras show the 9.7 and 20μm silicate emission. Recently, Vardya, de Jong & Willems (1986; hereafter VDJW) discovered using IRAS LRS spectra a weak broad emission feature ~12μm; this new feature may be silicate (VDJW). Here we investigate whether this can be due to H2O ice.
- Type
- Circumstellar Shells and Envelopes
- Information
- Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 221 - 222
- Copyright
- Copyright © Reidel 1987