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A First Study of Giant Stars in the Galactic Bulge based on Crires spectra
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Theoretical Astrophysics. (Teoretisk astrofysik)
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics. Department of Physics and Astronomy, Theoretical Astrophysics. (Teoretisk astrofysik)
Department of Physics and Astronomy, Theoretical Astrophysics. (Teoretisk astrofysik)
2007 (English)In: Stellar Populations as Building Blocks of Galaxies: Proceedings of IAU Symposium #241, 2007, 260-261 p.Conference paper, Published paper (Other scientific)
Abstract [en]

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.

Place, publisher, year, edition, pages
2007. 260-261 p.
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-13566DOI: doi:10.1017/S1743921307008113OAI: oai:DiVA.org:uu-13566DiVA: diva2:41336
Available from: 2008-01-23 Created: 2008-01-23

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Publisher's full texthttp://www.journals.cambridge.org/action/displayAbstract?fromPage=online&aid=1310084

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Ryde, NilsEdvardsson, BengtGustafsson, Bengt

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