NuSTAR and XMM-Newton Observations of the Neutron Star X-Ray Binary 1RXS J180408.9-34205
Harrison, F. A.; Fabian, A. C.; Miller, J. M.; Tomsick, J. A.; Bachetti, M.; Cackett, E. M.; Natalucci, L.; Barret, D.; Parker, M. L.; Rana, V.; Ludlam, R. M.
United States, United Kingdom, Italy, France, Germany
Abstract
We report on observations of the neutron star (NS) residing in the low-mass X-ray binary 1RXS J180408.9-34205 taken 2015 March by NuSTAR and XMM-Newton while the source was in the hard spectral state. We find multiple reflection features (Fe {{{K}}}α detected with NuSTAR; N vii, O vii, and O viii detected in the RGS) from different ionization zones. Through joint fits using the self-consistent relativistic reflection model relxill, we determine the inner radius to be ≤11.1 R g . For a 1.4 {M}⊙ NS with a spin of {a}\ast =0, this is an inner disk radius of ≤slant 22.2 km. We find the inclination of the system to be between 18° and 29°. If the disk is truncated at a radius greater than the NS radius, it could be truncated by a boundary layer on the NS surface. It is also possible that the disk is truncated at the magnetospheric radius; conservative estimates would then imply B≤slant (0.3{--}1.0)× {10}9 G at the magnetic poles, though coherent pulsations have not been detected and the source is not identified as a pulsar.