Stellar and wind properties of massive stars in the central parsec of the Galaxy
F. MartinsMax-Planck Institt fr extraterrestrische Physik, Postfach-1312, 85741, Garching, Germany e-mail: [email protected]R. GenzelDepartment of Physics, University of California, Berkeley, CA 94720, USAD. J. HillierDepartment of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara St., Pittsburgh, PA 15260, USAF. EisenhauerMax-Planck Institt fr extraterrestrische Physik, Postfach-1312, 85741, Garching, Germany e-mail: [email protected]T. PaumardLESIA, Observatoire de Paris, 5 Place Jules Janssen, 92195, Meudon, FranceS. GillessenMax-Planck Institt fr extraterrestrische Physik, Postfach-1312, 85741, Garching, Germany e-mail: [email protected]Thomas OttMax-Planck Institt fr extraterrestrische Physik, Postfach-1312, 85741, Garching, Germany e-mail: [email protected]Sascha TrippeMax-Planck Institt fr extraterrestrische Physik, Postfach-1312, 85741, Garching, Germany e-mail: [email protected]
2007en
ABI
Annotatsiya
Context.How star formation proceeds in the Galactic Center is a debated question. Addressing this question will help us understand the origin of the cluster of massive stars near the supermassive black hole, and more generally, starburst phenomena in galactic nuclei. In that context, it is crucial to know the properties of young massive stars in the central parsec of the Galaxy.
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