{"paper":{"title":"Suzaku Observation of GRS 1915+105: Evolution of Accretion Disc Structure during Limit-Cycle Oscillation","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"(2) Hiroshima University, (3) University of Durham, (4) Aoyama Gakuin University, (5) Physical Research Laboratory (6) Ehime University, (7) ISAS/JAXA, (8) CEA-Saclay), C. Done (3), H. Awaki (6), H. Shirai (2), H. Takahashi (2), J. Rodriguez (8), K. Ebisawa (7), K. Honda (2), K. Yamaoka (4), S. Chaty (8) ((1) Kyoto University, S. Naik (5), Y. Fukazawa (2), Y. Ueda (1)","submitted_at":"2010-03-01T11:41:13Z","abstract_excerpt":"We present results from the Suzaku observation of the microquasar GRS 1915+105 performed during the 2005 October multiwavelength campaign. The data include both stable state (class \\chi) and limit-cycle oscillation (class \\theta). Correct interstellar absorption as well as effects of dust scattering are fully taken into account in the spectral analysis. The energy spectra in the 2-120 keV band in both states are all dominated by strong Comptonization of disk photons by an optically thick (\\tau ~7-10) and low temperature (T_e ~2-3 keV) hybrid plasmas containing non-thermal electrons produced wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.0317","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}