Summary of IAU GA SpS 5 II: Stellar and Wind Parameters

(10) University of Amsterdam; (11) National Central University; (2) MPA Garching; (3) Armagh Observatory; (4) University of Sheffield; (5) University of Potsdam; (6) CSIC-INTA; (7) University of Erlangen-Nuremberg; (8) Ventspils University College; (9) Chinese Academy of Science

arxiv: 1210.4280 · v1 · pith:BEDO7PNJnew · submitted 2012-10-16 · 🌌 astro-ph.SR

Summary of IAU GA SpS 5 II: Stellar and Wind Parameters

F. Martins (1) , M. Bergemann (2) , J.M. Bestenlehner (3) , P.A. Crowther (4) , W.R. Hamann (^5) , F. Najarro (6) , M.F. Nieva (7) , N. Przybilla (7)

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J. Freimanis (8) W. Hou (9) L. Kaper (10) C.-D. Lee (11) ((1) LUPM (2) MPA Garching (3) Armagh Observatory (4) University of Sheffield (5) University of Potsdam (6) CSIC-INTA (7) University of Erlangen-Nuremberg (8) Ventspils University College (9) Chinese Academy of Science (10) University of Amsterdam (11) National Central University Taiwan)

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keywords infraredmassivestarsstellarwindaddressedadvantageavailable

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The development of infrared observational facilities has revealed a number of massive stars in obscured environments throughout the Milky Way and beyond. The determination of their stellar and wind properties from infrared diagnostics is thus required to take full advantage of the wealth of observations available in the near and mid infrared. However, the task is challenging. This session addressed some of the problems encountered and showed the limitations and successes of infrared studies of massive stars.

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Summary of IAU GA SpS 5 II: Stellar and Wind Parameters

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