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Results 1 - 4 of 4

Can Population III stars be major origins of both merging binary black holes and extremely metal poor stars?. (arXiv:2202.00230v1 [astro-ph.HE])
- Volume 17, Issue 5 - article #2
- Ataru Tanikawa, Gen Chiaki, Tomoya Kinugawa, Yudai Suwa, Nozomu Tominaga
- http://arxiv.org/abs/2202.00230
Long gamma-ray burst rate at very high redshift. (arXiv:1901.03516v1 [astro-ph.HE])
- Volume 14, Issue 3 - article #6
- Tomoya Kinugawa, Yuichi Harikane, Katsuaki Asano
- http://arxiv.org/abs/1901.03516
How to confirm the existence of population III stars by observations of gravitational waves. (arXiv:1709.08437v1 [astro-ph.HE])
- Volume 12, Issue 39 - article #4
- Akinobu Miyamoto, Tomoya Kinugawa, Takashi Nakamura, Nobuyuki Kanda
- http://arxiv.org/abs/1709.08437
Possible indirect confirmation of the existence of Pop III massive stars by gravitational wave
- Volume 9, Issue 20 - article #162
- Tomoya Kinugawa, Kohei Inayoshi, Kenta Hotokezaka, Daisuke Nakauchi, and Takashi Nakamura
- Monthly Notices of the Royal Astronomical Society - Volume: 442, Issue: 4
- Abstract Full Text (HTML) Full Text (PDF)

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