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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

Fabrice Martins ,
Reinhard Genzel ,
Frank Eisenhauer ,
Thibaut Paumard ,
Thomas Ott ,
Sascha Trippe  and
Stefan Gillessen
Fabrice Martins
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Reinhard Genzel
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Frank Eisenhauer
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Thibaut Paumard
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Thomas Ott
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Sascha Trippe
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
Stefan Gillessen
Affiliation:
MPE, Postfach 1312, D-85741 Garching bei München, Germany email: [email protected]
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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.

Keywords

stars: atmospheres stars: early-type stars: Wolf-Rayet Galaxy: center
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

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Najarro, F., Krabbe, A., Genzel, R., et al. 1997, A&A, 325, 700Google Scholar
Paumard, T., Genzel, R., Martins, F., et al. 2006, ApJ, 643, 1011CrossRefGoogle Scholar