Does the chemical signature of TYC 8442-1036-1 originate from a rotating massive star that died in a faint explosion?
Context. We have recently investigated the origin of chemical signatures observed in Galactic halo stars by means of a stochastic chemical evolution model. We have found that rotating massive stars are a promising way to explain several signatures observed in these fossil stars. Aims. In the present...
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| Main Authors: | , |
|---|---|
| Format: | Article (Journal) Chapter/Article |
| Language: | English |
| Published: |
August 12, 2016
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| In: |
Arxiv
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| Online Access: | Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1608.03455
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| Author Notes: | G. Cescutti, M. Valentini, P. François, C. Chiappini, E. Depagne, N. Christlieb, and C. Cortés |
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