IRAS and cool stellar mass loss

C. J. Skinner; B. Whitmore

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https://doi.org/10.1...arrow_drop_down

https://doi.org/10.1007/3-540-...

Part of book or chapter of book . 2008 . Peer-reviewed

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https://dx.doi.org/10.1007/3-5...

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IRAS and cool stellar mass loss

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type 07 Apr 2008 English Publisher:Springer Berlin Heidelberg

Authors: C. J. Skinner; B. Whitmore;

doi: 10.1007/3-540-18653-0_161

IRAS and cool stellar mass loss

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Abstract

We show that the band strength of the 9.7μm silicate dust feature is well correlated with the CO and OH-maser line strengths, and so provides a reliable measure of mass-loss rates for cool, luminous, Oxygen-rich stars. Correlations are presented between mass-loss rates and various physical properties of the M-Supergiants in the IRAS LRS Catalogue.

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University College London
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