@inproceedings{oai:jaxa.repo.nii.ac.jp:00005025,
 author = {牧島, 一夫 and Makishima, Kazuo},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, A fair fraction of Galactic stellar-mass black holes are reported to be rapidly spinning, based on their broad Fe-K lines. However, such broad features couple strongly with the spectral continuum, and cause the modeling to degenerate. By carefully analyzing broad-band Suzaku data, and also employing the information on optically-thick disk emission, GX 339-4 is inferred to harbor a low-spin black hole. In addition, the Suzaku spectra of the Seyfert galaxy MCG-6-30-15 are interpreted in an alternative way, without invoking the rapid black-hole spin., Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, 資料番号: AA0064574093, レポート番号: JAXA-SP-09-008E},
 pages = {252--255},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Continua and Iron-K Lines from Accreting Black Holes},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}