High-Resolution X-Ray Spectroscopy of the Bursting Pulsar GRO J1744-28
N. Degenaar, J.M. Miller, F.A. Harrison, J.A. Kennea, C. Kouveliotou,, G. Younes

TL;DR
This study uses high-resolution X-ray spectroscopy to analyze the accretion environment of the bursting pulsar GRO J1744-28, revealing a truncated disk, a strong magnetic field, and a fast disk wind, providing insights into neutron star accretion physics.
Contribution
First high-resolution spectral analysis of GRO J1744-28 revealing disk truncation, magnetic field strength, and disk wind characteristics.
Findings
Disk is truncated at ~85 GM/c^2.
Magnetic field estimated at (2-6)×10^10 G.
Detected fast disk wind with outflow velocity ~7500-8200 km/s.
Abstract
The bursting pulsar GRO J1744-28 is a Galactic low-mass X-ray binary that distinguishes itself by displaying type-II X-ray bursts: brief, bright flashes of X-ray emission that likely arise from spasmodic accretion. Combined with its coherent 2.1 Hz X-ray pulsations and relatively high estimated magnetic field, it is a particularly interesting source to study the physics of accretion flows around neutron stars. Here we report on Chandra/HETG observations obtained near the peak of its bright 2014 accretion outburst. Spectral analysis suggests the presence of a broad iron emission line centered at E_l ~ 6.7 keV. Fits with a disk reflection model yield an inclination angle of i ~ 52 degrees and an inner disk radius of R_in ~ 85 GM/c^2, which is much further out than typically found for neutron star low-mass X-ray binaries. Assuming that the disk is truncated at the magnetospheric radius of…
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