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Resolved Stellar Halos of M87 and NGC 5128: Metallicities from the Red-Giant Branch

Published online by Cambridge University Press:  09 May 2016

Sarah A. Bird*
Affiliation:
LAMOST Fellow, Shanghai Astronomical Observatory, 80 Nandan Road, Shanghai, 200030, China, email: [email protected]
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Abstract

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We have searched halo fields of two giant elliptical galaxies: M87, using HST images at 10 kpc from the galactic center, and NGC 5128 (Cen A), using VIMOS VLT images at 65 kpc from the center and archival HST data from 8 to 38 kpc from the center. We have resolved thousands of red-giant-branch (RGB) stars in these stellar halo fields using V and I filters, and, in addition, measured the metallicity using stellar isochrones. The metallicity distribution function (MDF) of the inner stellar halo of M87 is similar to that of NGC 5128's stellar halo.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Bird, S., Harris, W. E., Blakeslee, J. P., & Flynn, C. 2010, A&A, 524, A71Google Scholar
Bird, S. A., Flynn, C., Harris, W. E., & Valtonen, M. 2015, A&A, 575, A72Google Scholar
Harris, G. L. H., & Harris, W. E. 2000, AJ, 120, 2423Google Scholar
Harris, G. L. H., Harris, W. E., & Poole, G. B. 1999, AJ, 117, 855CrossRefGoogle Scholar
Harris, W. E., & Harris, G. L. H. 2002, AJ, 123, 3108Google Scholar
Rejkuba, M., Greggio, L., Harris, W. E., Harris, G. L. H., & Peng, E. W. 2005, ApJ, 631, 262Google Scholar