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Luminosities and mass-loss rates of carbon stars in the Magellanic Clouds
Authors:M A T Groenewegen  P R Wood  G C Sloan  J A D L Blommaert  M-R L Cioni  M W Feast  S Hony †  M Matsuura  J W Menzies  E A Olivier  E Vanhollebeke  J Th van Loon  P A Whitelock  A A Zijlstra  H J Habing  E Lagadec
Institution:Institute of Astronomy, University of Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium;Research School of Astronomy and Astrophysics, Australian National University, Cotter Road, Weston Creek, ACT 2611, Australia;Department of Astronomy, Cornell University, 108 Space Sciences Building, Ithaca, NY 14853-6801, USA;SUPA, School of Physics, University of Edinburgh, IFA, Blackford Hill, Edinburgh EH9 3HJ;Astronomy Department, University of Cape Town, 7701 Rondebosch, South Africa;APS Division, Department of Pure and Applied Physics, Queen's University Belfast, University Road BT7 1NN;National Astronomical Observatory of Japan, Osawa 2-21-1, Mitaka, Tokyo 181-8588, Japan;Astrophysics Group, School of Physical and Geographical Sciences, Keele University, Staffordshire ST5 5BG;School of Physics and Astronomy, University of Manchester, Sackville Street, PO Box 88, Manchester M60 1QD;South African Astronomical Observatory, PO Box 9, 7935 Observatory, South Africa;NASSP, Department of Mathematics and Applied Mathematics, University of Cape Town, 7701 Rondebosch, South Africa;Sterrewacht Leiden, Niels Bohrweg 2, 2333 RA Leiden, The Netherlands
Abstract:
Keywords:circumstellar matter  stars: AGB and post-AGB  stars: mass-loss  Magellanic Clouds  infrared: stars
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