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- W3098477569 abstract "At the distance of NGC 5128 ( Mpc) it is possible to resolve globular clusters with high resolution imaging from the ground, thus allowing the globular cluster candidate selection primarily through their morphological properties. I report the discovery of 71 globular clusters in NGC 5128 on VLT UT1+FORS1 images, including the faintest members () known to date in this galaxy as well as in 5 previously-known clusters. U- and V-band photometry has been measured for all the candidates and the luminosity function, spanning and , constructed. These are the deepest globular cluster luminosity functions in an elliptical galaxy determined so far. The Kolmogorov-Smirnov statistics show that the difference between the globular cluster luminosity functions of NGC 5128 and the MW is not larger than the difference between the ones of M 31 and the MW. The ()0 color histogram shows a bimodal distribution. For 23 globular clusters I obtained K-band images with SOFI at the NTT in La Silla. Their positions in the () vs. () color-color diagram indicate that they are indeed old globular clusters. Assuming that the globular clusters in NGC 5128 span a similar age range as the ones in the Milky Way and adopting a linear fit between the metallicity and ()0 color, the metal-rich clusters peak at dex and the metal-poor ones peak at dex." @default.
- W3098477569 created "2020-11-23" @default.
- W3098477569 creator A5001308404 @default.
- W3098477569 date "2001-04-01" @default.
- W3098477569 modified "2023-10-13" @default.
- W3098477569 title "Deep VLT search for globular clusters in NGC 5128: Color-magnitude diagrams and globular cluster luminosity function" @default.
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- W3098477569 doi "https://doi.org/10.1051/0004-6361:20010180" @default.
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