Abstract
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. © 2007 International Astronomical Union.
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APA
Martins, F., Genzel, R., Eisenhauer, F., Paumard, T., Ott, T., Trippe, S., & Gillessen, S. (2006). Stellar and wind properties of massive stars in the central parsec of the Galaxy. In Proceedings of the International Astronomical Union (Vol. 2, p. 207). Cambridge University Press. https://doi.org/10.1017/S1743921307010198
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