Home List of Titles Metallicity gradients at large galactocentric radii using the near-infrared Calcium triplet
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/73393
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- Metallicity gradients at large galactocentric radii using the near-infrared Calcium triplet
- Foster, Caroline; Proctor, Robert N.; Forbes, Duncan A.; Spolaor, Max; Hopkins, Philip F.; Brodie, Jean P.
- We describe a new spectroscopic technique for measuring radial metallicity gradients out to large galactocentric radii. We use the DEep Imaging Multi-Object Spectrograph (DEIMOS) on the Keck telescope and the galaxy spectrum extraction technique of Proctor et al. We also make use of the metallicity sensitive near-infrared Calcium ii triplet (CaT) features together with single stellar population models to obtain metallicities. Our technique is applied as a pilot study to a sample of three relatively nearby (≤30 Mpc) intermediate-mass to massive early-type galaxies. Results are compared with previous literature inner region values and generally show good agreement. We also include a comparison with profiles from dissipational disc–disc major merger simulations. Based on our new extended metallicity gradients combined with other observational evidence and theoretical predictions, we discuss possible formation scenarios for the galaxies in our sample. The limitations of our new technique are also discussed.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Monthly Notices of the Royal Astronomical Society, Vol. 400, no. 4 (Dec 2009), pp. 2135-2146
- Publication year
- Galaxy haloes; Large galactocentric radii; NGC 1407; NGC 2768; NGC 4494; Radial metallicity gradients; Spectroscopic techniques
- Wiley-Blackwell Publishing
- Publisher URL
- Copyright © 2009 The Authors. Journal compilation copyright © 2009 Royal Astronomical Society. The accepted manuscript of this paper is reproduced here in accordance with the copyright policy of the publisher. The definitive publication is available at www.interscience.wiley.com.
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