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A First Study of Giant Stars in the Galactic Bulge based on Crires spectra

Published online by Cambridge University Press:  01 December 2006

N. Ryde ,
B. Edvardsson ,
B. Gustafsson  and
H.-U. Käufl
N. Ryde
Affiliation:
Department of Astronomy and Space Physics, Uppsala University, Sweden email: [email protected], [email protected], [email protected]
B. Edvardsson
Affiliation:
Department of Astronomy and Space Physics, Uppsala University, Sweden email: [email protected], [email protected], [email protected]
B. Gustafsson
Affiliation:
Department of Astronomy and Space Physics, Uppsala University, Sweden email: [email protected], [email protected], [email protected]
H.-U. Käufl
Affiliation:
ESO, Garching, Germany email: [email protected]
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Abstract

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We present our on-going work on the determination of elemental abundances of giants in the Galactic Bulge by means of infrared spectroscopy. We show a preliminarily reduced spectrum and a synthetic spectrum fit of the Bulge giant Arp 4203 recorded with the near-infrared, high-resolution Crires spectrograph mounted on the VLT during its science verification run in August 2006. Abundances derived from this spectrum are discussed.

Keywords

stars: abundancesstars: individual (Arp 4203)Galaxy: bulgeinfrared: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 260 - 261
Copyright
Copyright © International Astronomical Union 2007

References

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Ryde, N., Gustafsson, B., Eriksson, K., & Wahlin, R. 2005, in ‘HR IR Spectroscopy in Astronomy’, ed. Käufl, H. U., Siebenmorgen, R., & Moorwood, A. F. M. (Springer), 365Google Scholar