{ "id": "1505.07112", "version": "v1", "published": "2015-05-26T20:00:30.000Z", "updated": "2015-05-26T20:00:30.000Z", "title": "A NuSTAR observation of disk reflection from close to the neutron star in 4U 1608-52", "authors": [ "N. Degenaar", "J. M. Miller", "D. Chakrabarty", "F. Harrison", "E. Kara", "A. C. Fabian" ], "comment": "5 pages, 4 figures, 1 table, MNRAS Letters in press", "categories": [ "astro-ph.HE" ], "abstract": "Studying the reflection of X-rays off the inner edge of the accretion disk in a neutron star low-mass X-ray binary, allows us to investigate the accretion geometry and to constrain the radius of the neutron star. We report on a NuSTAR observation of 4U 1608-52 obtained during a faint outburst in 2014 when the neutron star, which has a known spin frequency of 620 Hz, was accreting at ~1-2% of the Eddington limit. The 3-79 keV continuum emission was dominated by a Gamma~2 power law, with a ~1-2% contribution from a kTbb~0.3-0.6 keV black body component. The high-quality NuSTAR spectrum reveals the hallmarks of disk reflection; a broad iron line peaking near 7~keV and a Compton back-scattering hump around ~20-30 keV. Modeling the disk reflection spectrum points to a binary inclination of i~30-40 degrees and a small `coronal' height of h<8.5 GM/c2. Furthermore, our spectral analysis suggests that the inner disk radius extended to Rin~7-10 GM/c2, close to the innermost stable circular obit. This constrains the neutron star radius to R<21 km and the redshift from the stellar surface to z>0.12, for a mass of M=1.5 Msun and a spin parameter of a=0.29.", "revisions": [ { "version": "v1", "updated": "2015-05-26T20:00:30.000Z" } ], "analyses": { "keywords": [ "nustar observation", "neutron star low-mass x-ray binary", "kev black body component", "disk reflection spectrum points", "kev continuum emission" ], "publication": { "doi": "10.1093/mnrasl/slv072" }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1373264 } } }