Observations of a black hole x-ray binary indicate formation of a magnetically arrested disk.

Accretion of material onto a black hole drags any magnetic fields present inwards, increasing their strength. Theory predicts that sufficiently strong magnetic fields can halt the accretion flow, producing a magnetically arrested disk (MAD). We analyzed archival multiwavelength observations of an outburst from the black hole x-ray binary MAXI J1820+070 in 2018. The radio and optical fluxes were delayed compared with the x-ray flux by about 8 and 17 days, respectively. We interpret this as evidence for the formation of a MAD. In this scenario, the magnetic field is amplified by an expanding corona, forming a MAD around the time of the radio peak. We propose that the optical delay is due to thermal viscous instability in the outer disk.

A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism.

The megajansky radio burst, FRB 20200428, and other bright radio bursts detected from the Galactic source SGR J1935+2154 suggest that magnetars can make fast radio bursts (FRBs), but the emission site and mechanism of FRB-like bursts are still unidentified. Here, we report the emergence of a radio pulsar phase of the magnetar 5 months after FRB 20200428. Pulses were detected in 16.5 hours over 13 days using the Five-hundred-meter Aperture Spherical radio Telescope, with luminosities of about eight decades fainter than FRB 20200428. The pulses were emitted in a narrow phase window anti-aligned with the x-ray pulsation profile observed using the x-ray telescopes. The bursts, conversely, appear in random phases. This dichotomy suggests that radio pulses originate from a fixed region within the magnetosphere, but bursts occur in random locations and are possibly associated with explosive events in a dynamically evolving magnetosphere. This picture reconciles the lack of periodicity in cosmological repeating FRBs within the magnetar engine model.

Subsecond periodic radio oscillations in a microquasar.

Powerful relativistic jets are one of the ubiquitous features of accreting black holes in all scales1-3. GRS 1915 + 105 is a well-known fast-spinning black-hole X-ray binary4 with a relativistic jet, termed a 'microquasar', as indicated by its superluminal motion of radio emission5,6. It has exhibited persistent X-ray activity over the last 30 years, with quasiperiodic oscillations of approximately 1-10 Hz (refs. 7-9) and 34 and 67 Hz in the X-ray band10. These oscillations probably originate in the inner accretion disk, but other origins have been considered11. Radio observations found variable light curves with quasiperiodic flares or oscillations with periods of approximately 20-50 min (refs. 12-14). Here we report two instances of approximately 5-Hz transient periodic oscillation features from the source detected in the 1.05- to 1.45-GHz radio band that occurred in January 2021 and June 2022. Circular polarization was also observed during the oscillation phase.

Visible light transmittance of micro-pore optic plates for the wide-field x-ray telescope on the Einstein probe.

Micro-pore optics (MPO) has been employed in space x-ray telescopes for large field-of-view observations. For x-ray focal plane detectors with visible photon sensing capability, the optical blocking filter (OBF) on MPO devices is critical for preventing signal contamination by those photons. In this work, we designed a piece of equipment to measure the light transmission with high accuracy. The transmittance test results of the MPO plates meet the design requirements of less than 5×10-4. Based on the multilayer homogeneous film matrix method, we estimated possible combinations of film thicknesses (with alumina) that show a good agreement with the OBF design.

Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070.

A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each other. However, such an evolution is still unclear in both its geometry and dynamics. Here we report the unusual decrease of the reflection fraction in MAXI J1820+070, which is the ratio of the coronal intensity illuminating the disk to the coronal intensity reaching the observer, as the corona is observed to contrast during the decay phase. We postulate a jet-like corona model, in which the corona can be understood as a standing shock where the material flowing through. In this dynamical scenario, the decrease of the reflection fraction is a signature of the corona's bulk velocity. Our findings suggest that as the corona is observed to get closer to the black hole, the coronal material might be outflowing faster.

Inhibition of myeloid differentiation factor 88 signaling mediated by histidine-grafted poly(ß-amino ester) ester nanovector induces donor-specific liver allograft tolerance.

Toll-like receptors (TLRs) activate biochemical pathways that evoke activation of innate immunity, which leads to dendritic cell maturation and initiation of adaptive immune responses that provoke allograft rejection. We aimed to prolong allograft survival by selectively inhibiting expression of myeloid differentiation factor 88 (MyD88), which is an essential adaptor in TLR signaling. We designed and synthesized a novel histidine-grafted poly(ß-amino ester) (HGPAE) nanovector, which was shown to be safe and efficient both in vitro and in vivo for the delivery of a plasmid containing shRNA targeting MyD88 (pMyD88). We also demonstrated that the pMyD88/HGPAE complex mediated remarkable inhibition of MyD88 expression in rat liver in vivo. We transplanted Dark Agouti rat livers lacking MyD88 as result of transfection with the pMyD88/HGPAE complex into Lewis rats. The recipients survived longer and graft rejection of the donor liver as well as serum levels of IL-2 and IFN-γ in the recipient were significantly reduced.

pH- and reduction-responsive polymeric lipid vesicles for enhanced tumor cellular internalization and triggered drug release.

Enhanced tumor cellular internalization and triggered drug release are two main concerns in the development of nanoparticles for antitumor drug delivery. In this article, a new kind of smart pH- and reduction-dual-responsive drug- loaded PEG coated polymeric lipid vesicle (PPLV) that can achieve both enhanced tumor cellular internalization and triggered drug release has been designed and prepared. The PPLVs were formed from amphiphilic dextran derivatives. The antitumor drug, doxorubicin (DOX), was loaded in the cores of the PPLVs. The newly developed PPLVs had a nanosized structure (∼40 nm) with PEG coating, so they were neutral and had high colloidal stability in the blood circulation. The in vitro physicochemical characterizations showed that the PPLVs lose their PEG coating and expose the positive surface charge under acidic environments. The in vitro cellular uptake study indicated that the acidic-treated PPLVs can efficiently enter tumor cells. It has been demonstrated by in vitro DOX release profiles that the PPLVs can achieve a triggered drug release in response to the reduction environment. The MTT assay demonstrated that DOX-loaded PPLVs treated with pH 5.0 solution had higher antitumor activity than DOX-loaded PPLVs treated with pH 7.4 solution. These results suggested that the PPLVs were promising nanoparticles for smart antitumor drug delivery applications.

PEGlated magnetic polymeric liposome anchored with TAT for delivery of drugs across the blood-spinal cord barrier.

Due to the existence of the blood-spinal cord barrier (BSCB), many therapeutic macromolecular agents, such as drugs, protein and gene, cannot pass through this barrier to reach the site of injury, all of which restricts the treatment of spinal cord injuries (SCI). In this study, TAT-conjugated PEGlated Magnetic polymeric liposomes (TAT-PEG-MPLs) formed from PEGlated amphiphilic octadecyl quaternized carboxymethyl chitosan (PEG-OQCMC), cholesterol (Chol), superparamagnetic nanoparticles, and transactivating-transduction protein (TAT), were prepared successfully and evaluated the properties in vitro and in vivo. The result indicated that TAT-PEG-MPLs were spherical in solution, with significantly small mean diameter (83.2 nm) and excellent magnetism (magnetization saturation values of 43.5 emu/g). In vitro experiment, the uptake of PEG-MPLs with TAT by MCF-7 cells was greater than that of the PEG-MPLs without TAT. Most importantly, in vivo experiment, a low MRI signal was observed in the T(2)-weighted images; Histological analysis, Cryo-TEM and flame atomic absorption spectrophotometry revealed that TAT-PEG-MPLs nanoparticles significantly accumulated around the site of the SCI even inside the nerve cells. These nanoparticles may provide a promising carrier to locate to the lesion site, deliver therapeutic macromolecular agents across the BSCB and penetrate into the nerve cells for the treatment of SCI.