Gilmore, G. and Seabroke, G.
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RAVE (RAdial Velocity Experiment) is an ambitious international collaboration (PI: Matthias Steinmetz), using 6dF on the 1.2-m UK Schmidt Telescope at the Anglo-Australian Observatory, measuring the radial velocities, metallicities and abundance ratios of a large sample of stars (9 < I < 12) over the southern and equatorial sky. The RAVE observing campaign began in April 2003 and to date 50,000 spectra have been obtained. We are analysing RAVE's first year unpublished data (30,000 stars) specifically to quantify the kinematics of the Galactic thick disk. We present our first RAVE statistical study of the local thick disk, using reduced proper motion diagrams in addition to our radial velocity data.
|Item Type:||Conference Item|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||George Seabroke|
|Date Deposited:||04 Feb 2009 06:15|
|Last Modified:||04 Oct 2016 10:17|
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