Abstract
High resolution spectral data of red clump stars towards the NGP have been obtained with the spectrograph Elodie at OHP stars. Nearby Hipparcos red clump stars were also observed. We determine the thin and thick properties: kinematics and chemical abundances in the solar neighbourhood. We estimate the surface mass density of the galactic disk, we also determine the thin and thick disk chemical properties.
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References
1. C. Soubiran, O. Bienaymé, A. Siebert: Astron. Astrophys. 398, 141 (2003)
2. A. Siebert, O. Bienaymé, C. Soubiran Astron. Astrophys. 399, 531 (2003)
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Bienaymé, O., Mishenina, T., Soubiran, C., Kovtyukh, V., Siebert, A. (2006). Chemical Composition and Kinematics of Disk Stars. In: Randich, S., Pasquini, L. (eds) Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-34136-9_11
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DOI: https://doi.org/10.1007/978-3-540-34136-9_11
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-34135-2
Online ISBN: 978-3-540-34136-9
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