The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars as Nucleosynthetic Probes of the Early Universe

@article{Nomoto2007TheCB,
  title={The Connection between Gamma-Ray Bursts and Extremely Metal-Poor Stars as Nucleosynthetic Probes of the Early Universe},
  author={Ken’ichi Nomoto and Nozomu Tominaga and M. Tanaka and Keiichi Maeda and Hideyuki Umeda},
  journal={Proceedings of the International Astronomical Union},
  year={2007},
  volume={3},
  pages={463 - 470}
}
Abstract The connection between the long GRBs and Type Ic Supernovae (SNe) has revealed the interesting diversity: (i) GRB-SNe, (ii) Non-GRB Hypernovae (HNe), (iii) X-Ray Flash (XRF)-SNe, and (iv) Non-SN GRBs (or dark HNe). We show that nucleosynthetic properties found in the above diversity are connected to the variation of the abundance patterns of extremely-metal-poor (EMP) stars, such as the excess of C, Co, Zn relative to Fe. We explain such a connection in a unified manner as… Expand

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