{ "id": "1810.07115", "version": "v1", "published": "2018-10-16T16:14:41.000Z", "updated": "2018-10-16T16:14:41.000Z", "title": "Study of the reflection spectra of SAX J1748.9-2021", "authors": [ "Rahul Sharma", "Chetana Jain", "Anjan Dutta" ], "comment": "6 pages, 6 figures. Accepted for publication in MNRAS", "doi": "10.1093/mnras/sty2808", "categories": [ "astro-ph.HE" ], "abstract": "We report the spectral analysis of accretion powered millisecond X-ray pulsar SAX J1748.9-2021 from the NuSTAR observation made during its 2015 outburst. The spectra displayed a broad emission line at $\\sim 6.5$ keV with line width of $\\sim 0.5$ keV and excess above $\\sim 20$ keV due to Compton hump. The persistent emission of SAX J1748.9-2021 is described by a combination of soft thermal component with $kT =0.62^{+0.03}_{-0.05}$ keV and thermally Comptonized component with $kT_e=2.50^{+0.06}_{-0.03}$ keV reflected from the disc with reflection fraction of $0.30^{+0.08}_{-0.04}$. We have modeled the reflection spectrum with self-consistent model relxillCP and have found the inclination of the accretion disc to be $32.3^{^\\circ +4.8}_{-4.7}$ and log $\\xi$ is equal to $3.05^{+0.40}_{-0.34}$. We have obtained an upper limit of 57 km for inner disc radius; and the estimated magnetic field strength at the poles is less than $3.4 \\times 10^9$ G. This kind of detailed investigation of reflection spectrum of SAX J1748.9-2021, especially above 10 keV, has been achieved only because of high statistics NuSTAR data of the source.", "revisions": [ { "version": "v1", "updated": "2018-10-16T16:14:41.000Z" } ], "analyses": { "keywords": [ "reflection spectrum", "millisecond x-ray pulsar sax j1748", "powered millisecond x-ray pulsar sax", "accretion powered millisecond x-ray pulsar", "high statistics nustar data" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }