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1.3. First stellar iron abundance measurements in the Galactic center

Published online by Cambridge University Press:  25 May 2016

K. Sellgren ,
J. S. Carr  and
S. C. Balachandran
K. Sellgren
Affiliation:
Ohio State University, Columbus, OH 43210 USA
J. S. Carr
Affiliation:
Naval Research Laboratory, Washington DC 20375 USA
S. C. Balachandran
Affiliation:
University of Maryland, College Park, MD 20742 USA

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The disk of the Milky Way galaxy shows evidence for gas-phase abundances which increase with decreasing radius (Simpson et al. 1995; Afflerbach et al. 1997). Sustained star formation in the center of the Milky Way Galaxy may be fueled by inflow of inner disk gas (Serabyn & Morris 1996), suggesting that Galactic Center (GC) stars may be metal-rich. Measurements of stellar abundances in the GC allow us to explore the chemical evolution of our Galaxy's nucleus and to infer its star formation history.

Type
Part I. Stellar Cluster, Star Formation
Information
Symposium - International Astronomical Union , Volume 184: The Central Regions of the Galaxy and Galaxies , 1998 , pp. 21 - 22
Copyright
Copyright © Kluwer 1998 

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