SpS5 - II. Stellar and wind parameters

  • 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.

Download full text files

  • SHA-1: a87d8ff163baf6cb7c29b4a957084bd89e867d0b

Export metadata

Additional Services

Share in Twitter Search Google Scholar Statistics
Author:Fabrice Martins, Maria Bergemann, Joachim M. Bestenlehner, Paul A. CrowtherORCiD, Wolf-Rainer HamannORCiDGND, Francisco Najarro, Maria Fernanda Nieva, Norbert Przybilla, Juris Freimanis, Weizhen Hou, Lex Kaper
Parent Title (German):Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe
Series (Serial Number):Postprints der Universität Potsdam : Mathematisch-Naturwissenschaftliche Reihe (688)
Document Type:Postprint
Date of first Publication:2019/04/08
Year of Completion:2012
Publishing Institution:Universität Potsdam
Release Date:2019/04/08
Tag:infrared: stars; stars: abundances; stars: early-type; stars: fundamental parameters; stars: late-type; stars: mass loss
Source:Highlights of Astronomy 16 (2012) DOI: 10.1017/S1743921314011788
Organizational units:Mathematisch-Naturwissenschaftliche Fakultät
Dewey Decimal Classification:5 Naturwissenschaften und Mathematik / 52 Astronomie
Peer Review:Referiert
Publication Way:Open Access
Grantor:Cambridge University Press (CUP)
Licence (German):License LogoKeine Nutzungslizenz vergeben - es gilt das deutsche Urheberrecht