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Orbitally modulated dust formation by the WC7+O5 colliding-wind binary WR 140
Authors:P M Williams  S V Marchenko  A P Marston  A F J Moffat  W P Varricatt  S M Dougherty  M R Kidger  L Morbidelli  M Tapia
Institution:Institute for Astronomy, Scottish Universities Physics Alliance, University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ;Department of Physics and Astronomy, Western Kentucky University, 1906 College Heights Blvd #11077, Bowling Green, KY 42101, USA;SIRTF Science Center, IPAC, Caltech, Mail Stop 314-6, Pasadena, CA 91125, USA;Herschel Science Centre, European Space Astronomy Centre, Villafranca del Castillo, PO Box - Apdo.50727, 28080 Madrid, Spain;Département de physique, Universitéde Montréal, C.P. 6128, Succ. Centre-Ville, Montréal, QC, H3C 3J7, Canada;Joint Astronomy Centre, 660 N. A'ohōkūPlace, Hilo, HI 96720, USA;National Research Council of Canada, Herzberg Institute for Astrophysics, Dominion Radio Astrophysical Observatory, PO Box 248, Penticton, B.C. V2A 6J9, Canada;Ingenieria y Servicios Aeroespaciales SA, ESAC, Villafranca del Castillo, PO Box - Apdo.50727, 28080 Madrid, Spain;INAF - Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy;Universidad Nacional Autónoma de México, Instituto de Astronomía, Apartado Postal 877, Ensenada B.C., Mexico
Abstract:
Keywords:circumstellar matter  stars: individual: WR 140  stars: Wolf-Rayet  infrared: stars
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