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globular clusters: individual (ω centauri)

Publications of the Astronomical Society of Australia (1)

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Observed Abundance Features and their Implications for Chemical Evolution
Takuji Tsujimoto, Toshikazu Shigeyama
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Publications of the Astronomical Society of Australia / Volume 21 / Issue 2 / 2004

Published online by Cambridge University Press:

05 March 2013, pp. 242-247
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We describe the star formation histories of the Milky Way dwarf spheroidal galaxy and the globular cluster ω Centauri in terms of an inhomogeneous chemical evolution model developed for the Galactic halo. The observed abundance trends seen in neutron-capture elements together with α-elements constrain our models to shed light on the histories of these nearby galaxies and ω Cen. The origin of low-α stars and a new picture of the globular cluster formation scenario induced by cloud–cloud collisions are also presented.