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天体物理学実習 II 関連資料

天体物理学実習 II 関連資料. Blackhole binary scales McClintock et al. 2011, arXiv:1101.0811. VLBA observation Parallax (1.86 kpc away) + orbital motion (5.6d) ? Reid et al. 2011, arXiv:1106.3688. Results of optical light curve modeling Companion 19.2Msolar, CygX-1 14.8 Msolar

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天体物理学実習 II 関連資料

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  1. 天体物理学実習 II 関連資料

  2. Blackhole binary scales McClintock et al. 2011, arXiv:1101.0811

  3. VLBA observation Parallax (1.86 kpc away) + orbital motion (5.6d) ? Reid et al. 2011, arXiv:1106.3688 Results of optical light curve modeling Companion 19.2Msolar, CygX-1 14.8 Msolar Orosz et al. 2011, arXiv:1106.3689

  4. Non-rotating Innermost Stable Circular Orbit (3Rs) SED modeling constrains the size of the Rin = r_ISCOwhich reflects spin-parameter a McClintock et al. 2011, arXiv:1101.0811

  5. Results of SED modeling of CygX-1 -> spin parameter a>0.91-0.97 ? Orosz et al. 2011, arXiv:1106.3689

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