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Luminosities and mass-loss rates of carbon stars in the Magellanic Clouds

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Authors

Groenewegen, M A T
Wood, Peter R
Sloan, G C
Blommaert, J A D L
Cioni, M-R L
Feast, M.W.
Hony, S
Matsuura, M.
Menzies, J. W
Olivier, E. A.

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Blackwell Publishing Ltd

Abstract

Dust radiative transfer models are presented for 60 carbon stars in the Magellanic Clouds (MCs) for which 5-35 μm Spitzer infrared spectrograph (IRS) spectra and quasi-simultaneous ground-based JHKL photometry are available. From the modelling, the lumin

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Monthly Notices of the Royal Astronomical Society

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Restricted until

2037-12-31
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