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

Groenewegen, M A TWood, Peter RSloan, G CBlommaert, J A D LCioni, M-R LFeast, M.W.Hony, SMatsuura, M.Menzies, J. WOlivier, E. A.Vanhollebeke, Evan Loon, Jacco ThWhitelock, Patricia AZijlstra, Albert AHabing, H.J.Lagadec, Eric2015-12-070035-8711http://hdl.handle.net/1885/18678Dust 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 luminKeywords: Circumstellar matter; Infrared: stars; Magellanic clouds; Stars: AGB and post-AGB; Stars: mass-lossLuminosities and mass-loss rates of carbon stars in the Magellanic Clouds200710.1111/j.1365-2966.2007.11428.x2015-12-07