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Stellar and wind properties of massive stars in the central parsec of the Galaxy
Published online by Cambridge University Press: 01 August 2006
Abstract
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The stellar and wind properties of the new population of massive stars in the central parsec of the Galaxy are derived through quantitative analysis with atmosphere models.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 207
- Copyright
- Copyright © International Astronomical Union 2007
References
Lutz, D. 1999, in: Cox, P. & Kessler, M. F. (eds.), The Universe as Seen by ISO, ESA SP-427, 623Google Scholar
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