Hasil Pencarian - Tomoaki Ishiyama

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  1. 1
    Halo Substructure Boosts to the Signatures of Dark Matter Annihilation

    Halo Substructure Boosts to the Signatures of Dark Matter Annihilation oleh Shin’ichiro Ando, Tomoaki Ishiyama, Nagisa Hiroshima

    Diterbitkan 2019-07-01
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  2. 2
    Theoretical Re-evaluations of Scaling Relations between SMBHs and Their Host Galaxies–2. Importance of AGN Feedback Suggested by Stellar Age–Velocity Dispersion Relation

    Theoretical Re-evaluations of Scaling Relations between SMBHs and Their Host Galaxies–2. Importance of AGN Feedback Suggested by Stellar Age–Velocity Dispersion Relation oleh Hikari Shirakata, Toshihiro Kawaguchi, Takashi Okamoto, Tomoaki Ishiyama

    Diterbitkan 2017-09-01
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  3. 3
    Dark Matter Halo Properties of the Galactic Dwarf Satellites: Implication for Chemo-dynamical Evolution of the Satellites and a Challenge to Lambda Cold Dark Matter

    Dark Matter Halo Properties of the Galactic Dwarf Satellites: Implication for Chemo-dynamical Evolution of the Satellites and a Challenge to Lambda Cold Dark Matter oleh Kohei Hayashi, Yutaka Hirai, Masashi Chiba, Tomoaki Ishiyama

    Diterbitkan 2023-01-01
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  4. 4
    Constraining Cosmological Parameters Using the Cluster Mass–Richness Relation

    Constraining Cosmological Parameters Using the Cluster Mass–Richness Relation oleh Mohamed H. Abdullah, Gillian Wilson, Anatoly Klypin, Tomoaki Ishiyama

    Diterbitkan 2023-01-01
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  5. 5
    Theoretical Re-evaluations of Scaling Relations between SMBHs and Their Host Galaxies—1. Effect of Seed BH Mass

    Theoretical Re-evaluations of Scaling Relations between SMBHs and Their Host Galaxies—1. Effect of Seed BH Mass oleh Hikari Shirakata, Toshihiro Kawaguchi, Takashi Okamoto, Ryu Makiya, Ryu Makiya, Tomoaki Ishiyama, Yoshiki Matsuoka, Masahiro Nagashima, Motohiro Enoki, Taira Oogi, Masakazu A. R. Kobayashi

    Diterbitkan 2017-09-01
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