{ "id": "1403.6739", "version": "v1", "published": "2014-03-26T16:37:38.000Z", "updated": "2014-03-26T16:37:38.000Z", "title": "To understand the X-ray spectrum of anomalous X-ray pulsars and soft gamma-ray repeaters", "authors": [ "Yan-Jun Guo", "Shi Dai", "Zhao-Sheng Li", "Yuan Liu", "Hao Tong", "Ren-Xin Xu" ], "comment": "12 pages, 6 figures, 6 tables, submitted to RAA", "categories": [ "astro-ph.HE" ], "abstract": "Hard X-rays above 10 keV are detected from several anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs), and different models have been proposed to explain the physical origin within the frame of either magnetar model or fallback disk system. Using data from $\\it Suzaku$ and INTEGRAL, we study the soft and hard X-ray spectra of four AXPs/SGRs, 1RXS J170849-400910, 1E 1547.0-5408, SGR 1806-20 and SGR 0501+4516. It is found that the spectra could be well reproduced by bulk-motion Comptonization (BMC) process as was first suggested by Tr$\\\"u$mper et al., showing that the accretion scenario could be compatible with X-ray emission of AXPs/SGRs. HXMT simulations for BMC model show that the spectra would have discrepancies from power-law, especially the cutoff at $\\sim$ 200 keV. Thus future observations are promising to distinguish different models for the hard tail and may help us understand the nature of AXPs/SGRs.", "revisions": [ { "version": "v1", "updated": "2014-03-26T16:37:38.000Z" } ], "analyses": { "keywords": [ "soft gamma-ray repeaters", "anomalous x-ray pulsars", "x-ray spectrum", "understand", "fallback disk system" ], "publication": { "doi": "10.1088/1674-4527/15/4/006", "journal": "Research in Astronomy and Astrophysics", "year": 2015, "month": "Apr", "volume": 15, "number": 4, "pages": 525 }, "note": { "typesetting": "TeX", "pages": 12, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1287330, "adsabs": "2015RAA....15..525G" } } }