The multi-wavelength view of Hot, Massive Stars: Concluding remarks

Details The multi-wavelength view of Hot, Massive Stars: Concluding remarks The multi-wavelength view of Hot, Massive Stars: Concluding remarks

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011bsrsl..80..739g&link_type=abstract

Société Royale des Sciences de Liège, Bulletin, vol. 80, p. 739-747 (Proceedings of the 39th Liège Astrophysical Colloquium, hel

Astronomy and Astrophysics

Astrophysics

Scientific paper

The papers in this volume demonstrate the importance of adopting a multi-wavelength approach to understanding hot, massive stars and their environments. They also reflect an excitement about recent developments in the field of massive star research that was so clearly evident during the meeting in Liège. Here I review some of the topics and results that were presented at the meeting that capture a sense of the emerging issues and opportunities in massive star studies.

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