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SpS5 - III. Matter ejection and feedback

Nazé, Yaël ; Che, Xiao ; Cox, Nick L. J. ; Groh, José H. ; Guerrero, Martin ; Kervella, Pierre ; Lee, Chien-De ; Matsuura, Mikako ; Oey, M. Sally ; Stringfellow, Guy S. ; Wachter, Stephanie ; Montmerle, Thierry

In: Proceedings of the International Astronomical Union, 2012, vol. 10, no. H16, p. 429-438

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    Titre
    • SpS5 - III. Matter ejection and feedback
    Auteur
    • Nazé, Yaël. Department AGO, Allée du 6 Août 17, B5C, 4000-Liège, Belgium, email: naze@astro.ulg.ac.be
    • Che, Xiao. Dpt of Astronomy, Univ. of Michigan, 830 Dennison Bldg, Ann Arbor, MI 48109-1042, USA
    • Cox, Nick L. J.. Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, Leuven, Belgium
    • Groh, José H.. Geneva Observ., Univ. of Geneva, Chemin des Maillettes 51, CH-1290 Sauverny, Switzerland
    • Guerrero, Martin. IAA-CSIC, Glorieta de la Astronomia s/n, 18008 Granada, Spain
    • Kervella, Pierre. LESIA, Obs. de Paris, CNRS UMR 8109, UPMC, 5 place J. Janssen, 92195, Meudon, France
    • Lee, Chien-De. Graduate institute of astronomy, National central university, Taiwan
    • Matsuura, Mikako. Department of Physics and Astronomy, UCL, Gower Street, London WC1E 6BT, UK
    • Oey, M. Sally. Dpt of Astronomy, Univ. of Michigan, 830 Dennison Bldg, Ann Arbor, MI 48109-1042, USA
    • Stringfellow, Guy S.. Center for Astroph. and Space Astr., Univ. of Colorado, 389 UCB, Boulder, CO, USA
    • Wachter, Stephanie. IPAC, California Inst. of Technology, Pasadena, CA 91125, USA
    • Montmerle, Thierry. 1 Department AGO, Allée du 6 Août 17, B5C, 4000-Liège, Belgium, email
    Type de document
    • Postprint
    Langue
    • Anglais
    Publié dans
    • Proceedings of the International Astronomical Union, 2012, vol. 10, no. H16, p. 429-438. Cambridge University Press
    Autre version électronique
    Identifiant OAI-PMH
    • oai:doc.rero.ch:302497
    Summary
    The last part of SpS5 dealt with the circumstellar environment. Structures are indeed found around several types of massive stars, such as blue and red supergiants, as well as WRs and LBVs. As shown in the last years, the potential of IR for their study is twofold: first, IR can help discover many previously unknown nebulae, leading to the identification of new massive stars as their progenitors; second, IR can help characterize the nebular features. Current and new IR facilities thus pave the way to a better understanding of the feedback from massive stars