Skip navigation
Skip navigation

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

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.; Vanhollebeke, E; van Loon, Jacco Th; Whitelock, Patricia A; Zijlstra, Albert A; Habing, H.J.; Lagadec, Eric


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

CollectionsANU Research Publications
Date published: 2007
Type: Journal article
Source: Monthly Notices of the Royal Astronomical Society
DOI: 10.1111/j.1365-2966.2007.11428.x


File Description SizeFormat Image
01_Groenewegen_Luminosities_and_mass-loss_2007.pdf3.29 MBAdobe PDF    Request a copy

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  19 May 2020/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator