EPJ Web of Conferences
Volume 19, 2012Assembling the Puzzle of the Milky Way
|Number of page(s)||3|
|Section||Inner Galaxy: Bulge/Bar/Inner Disc Interplay, Role of Mergers|
|Published online||07 February 2012|
Elemental abundances in AGB stars and the formation of the Galactic bulge
1 University of Vienna, Department of Astronomy, Türkenschanzstraße 17, 1180 Vienna, Austria
2 Instituut voor Sterrenkunde, K. U. Leuven, Celestijnenlaan 200D, 3000 Leuven, Belgium
3 Department of Astronomy and Theoretical Physics, Box 43, 22100 Lund, Sweden
4 Research School of Astronomy and Astrophysics, Australian National University, Cotter Rd, Weston Creek ACT 2611, Australia
5 Observatoire de Besanç on, 41bis, avenue de l’Observatoire, 25000 Besançon, France
6 INAF - Padova Astronomical Observatory, Vicolo dell’Osservatorio 5, 35122 Padova, Italy
a e-mail: email@example.com
We obtained high-resolution near-IR spectra of 45 AGB stars located in the Galactic bulge. The aim of the project is to determine key elemental abundances in these stars to help constrain the formation history of the bulge. A further aim is to link the photospheric abundances to the dust species found in the winds of the stars. Here we present a progress report of the analysis of the spectra.
© Owned by the authors, published by EDP Sciences, 2012
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.