Identification of the long stellar stream of the prototypical massive globular cluster ω Centauri
Author:
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Link
http://www.nature.com/articles/s41550-019-0751-x.pdf
Reference51 articles.
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2. Johnson, C. I. & Pilachowski, C. A. Chemical abundances for 855 giants in the globular cluster Omega Centauri (NGC 5139). Astrophys. J. 722, 1373–1410 (2010).
3. Bellini, A. et al. The HST large programme on Omega Centauri. II. Internal kinematics. Astrophys. J. 853, 86 (2018).
4. Marino, A. F. et al. The C+N+O abundance of Omega Centauri giant stars: implications for the chemical-enrichment scenario and the relative ages of different stellar populations. Astrophys. J. 746, 14 (2012).
5. Zinnecker, H., Keable, C. J., Dunlop, J. S., Cannon, R. D. & Griffiths, W. K. In The Harlow Shapley Symposium on Globular Cluster Systems in Galaxies (eds Grindlay, J. E. & Davis Philip, A. G.) 603–604 (IAU, 1988).
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