1 / 6

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

rowa
Télécharger la présentation

天体物理学実習 II 関連資料

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  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

More Related