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Spectropolarimetry of the massive post-red supergiants IRC +10420 and HD 179821
Authors:M Patel  R D Oudmaijer  J S Vink  J E Bjorkman  B Davies  M A T Groenewegen  A S Miroshnichenko  J C Mottram
Institution:School of Physics and Astronomy, University of Leeds, Woodhouse Lane, Leeds LS2 9JT;Astrophysics Group, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ;Armagh Observatory, College Hill, Armagh BT61 9DG;Lennard–Jones Laboratory, Astrophysics, Keele University, Keele ST5 5BG;Ritter Observatory, M.S. 113, Department of Physics and Astronomy, University of Toledo, Toledo, OH 43606-3390, USA;Chester F. Carlson Centre for Imaging Science, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623-5604, USA;Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200 D, 3001 Leuven, Belgium;Department of Physics and Astronomy, University of North Carolina at Greensboro, PO Box 26170, Greensboro NC 27402-6170, USA
Abstract:
Keywords:techniques: polarimetric  circumstellar matter  stars: evolution  stars: individual: IRC +10 420  stars: individual: HD 179 821
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