Simultaneous NICER and NuSTAR Observations of the Ultra-compact X-ray Binary 4U 1543-624
R. M. Ludlam, A. D. Jaodand, J. A. Garc\'ia, N. Degenaar, J. A., Tomsick, E. M. Cackett, A. C. Fabian, P. Gandhi, D. J. K. Buisson, A. W., Shaw, D. Chakrabarty

TL;DR
This study presents joint NuSTAR and NICER observations of the ultra-compact X-ray binary 4U 1543-624, analyzing its reflection features, disk radius, and magnetic field constraints to understand the accretion environment around the neutron star.
Contribution
First joint NuSTAR and NICER observations of 4U 1543-624 with detailed reflection modeling and constraints on the neutron star's magnetic field and radius.
Findings
Reflection features indicate a disk radius close to the innermost stable orbit.
Upper limit on magnetic field strength is 0.7×10^8 G.
Neutron star radius constrained to ≤12.1 km.
Abstract
We present the first joint NuSTAR and NICER observations of the ultra-compact X-ray binary (UCXB) 4U 1543624 obtained in 2020 April. The source was at a luminosity of ergs s and showed evidence of reflected emission in the form of an O VIII line, Fe K line, and Compton hump within the spectrum. We used a full reflection model, known as xillverCO, that is tailored for the atypical abundances found in UCXBs, to account for the reflected emission. We tested the emission radii of the O and Fe line components and conclude that they originate from a common disk radius in the innermost region of the accretion disk (). Assuming that the compact accretor is a neutron star (NS) and the position of the inner disk is the Alfv\'{e}n radius, we placed an upper limit on the magnetic…
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