Sub-second infrared variability from the archetypal accreting neutron star 4U 1728−34
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 525:2 (2023) 2509-2518
The accretion/ejection link in the neutron star X-ray binary 4U 1820-30 I: a boundary layer-jet coupling?
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 525:2 (2023) 2366-2379
First Detection of X-Ray Polarization from the Accreting Neutron Star 4U 1820−303
The Astrophysical Journal Letters American Astronomical Society 953:2 (2023) L22-L22
Abstract:
Low-mass X-ray binaries hosting weakly magnetized neutron stars (NS-LMXBs) are among the brightest sources in the X-ray sky. Since 2021, the Imaging X-ray Polarimetry Explorer (IXPE) has provided new measurements of the X-ray polarization of these sources. IXPE observations have revealed that most NS-LMXBs are significantly polarized in the X-rays, providing unprecedented insight into the geometry of their accretion flow. In this review paper, we summarize the first results obtained by IXPE on NS-LMXBs, the emerging trends within each class of sources (atoll/Z), and possible physical interpretations.8 pages, 3 figures, invited review for the Special Issue X-ray Polarization: A New Era BeginDiscovery of an extremely intermittent periodic radio source
Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 526:1 (2023) l143-l148
FRB 20121102A: images of the bursts and the varying radio counterpart
ArXiv 2308.04298 (2023)