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IR excess stars and shock filaments at the Galactic center

Published online by Cambridge University Press:  24 November 2004

J. Moultaka ,
A. Eckart ,
T. Viehmann ,
R. Schödel ,
N. Mouawad  and
C. Straubmeier
J. Moultaka
Affiliation:
Universität zu Köln, I. Physikalisches Institut, Zülpicher str. 77, 50937 Köln, Germany email: [email protected]
A. Eckart
Affiliation:
Universität zu Köln, I. Physikalisches Institut, Zülpicher str. 77, 50937 Köln, Germany email: [email protected]
T. Viehmann
Affiliation:
Universität zu Köln, I. Physikalisches Institut, Zülpicher str. 77, 50937 Köln, Germany email: [email protected]
R. Schödel
Affiliation:
Universität zu Köln, I. Physikalisches Institut, Zülpicher str. 77, 50937 Köln, Germany email: [email protected]
N. Mouawad
Affiliation:
Universität zu Köln, I. Physikalisches Institut, Zülpicher str. 77, 50937 Köln, Germany email: [email protected]
C. Straubmeier
Affiliation:
Universität zu Köln, I. Physikalisches Institut, Zülpicher str. 77, 50937 Köln, Germany email: [email protected]
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Abstract

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In this paper we report on our recent results connected with the direct environment of the super massive black hole of the Milky Way. The data are obtained using the VLT facilities (ISAAC and NAOS/CONICA instruments) in the near- and mid-infrared wavelength ranges. We provide a calibration of the foreground and local differential (in wavelength and spatially) extinction of the Galactic Center and report on the discovery of a new complex of infrared excess sources (possibly young stars) located at the northern part of the IRS 13 cluster. Finally, we discuss the origin of filamentary structures observed in the L-band images.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
ORAL CONTRIBUTIONS
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS222 , March 2004 , pp. 141 - 144
Copyright
© 2004 International Astronomical Union