Thermal and non-thermal X-ray emission from the rotation-powered radio/γ-ray pulsar PSR J1740+1000 [PDF]
Michela Rigoselli +6 more
openalex +1 more source
Stem cell spheroids, produced via a high‐throughput microfabrication technique, are transported within a vortex generated at the outlet channels of a cross‐slot millifluidic chip. For Reynolds number exceeding 170–200, intermittent high shear stresses applied to each spheroid within the vortex trigger a massive release of biologically active ...
Elliot Thouvenot +8 more
wiley +1 more source
Modeling X-Ray and Gamma-Ray Emission from Redback Pulsar Binaries
We investigated the multiband emission from the pulsar binaries XSS J12270−4859, PSR J2039−5617, and PSR J2339−0533, which exhibit orbital modulation in the X-ray and gamma-ray bands.
Minju Sim +2 more
doaj +1 more source
Insight-HXMT insight into switch of the accretion mode: the case of the X-ray pulsar 4U 1901+03 [PDF]
Y. L. Tuo +99 more
openalex +1 more source
Discovery of two cyclotron resonance scattering features in X-ray pulsar cen X-3 by Insight-HXMT [PDF]
Weiguo Yang +6 more
openalex +1 more source
STING Agonists and How to Reach Their Full Potential in Cancer Immunotherapy
STING agonists show promise in preclinical studies in boosting an anti‐tumor response using the immune system. However, different limitations remain, and future research is needed to better understand how STING activation impacts the tumor microenvironment, identify effective combination strategies, and determine the best tumor types for STING agonist ...
Laura Gehrcken +3 more
wiley +1 more source
NuSTAR and XMM-Newton Observations of PSR J1930+1852 and Its Pulsar Wind Nebula
Synchrotron X-ray emission from a pulsar wind nebula (PWN) is a sensitive probe of its magnetic field and high-energy particle population. Here we analyze contemporaneous NuSTAR and XMM - Newton observations of the PWN G54.1+0.3, powered by pulsar PSR ...
J. A. J. Alford +2 more
doaj +1 more source
High-energy Emission from the Intrabinary Shocks in Redback Pulsars
The intrabinary shocks (IBS) of spider pulsars emit nonthermal synchrotron X-rays from accelerated electrons and positrons in the shocked pulsar wind, likely energized by magnetic reconnection.
Andrew G. Sullivan, Roger W. Romani
doaj +1 more source
The Resonant Bremsstrahlung of Ultrarelativistic Electrons on a Nucleus with Radiation of Hard Gamma-Quanta in the Presence of a Pulsed Field of the X-ray Pulsar [PDF]
Alexander Dubov +2 more
openalex +1 more source
Spectral properties of the Be/X-ray pulsar 2S 1553-542 during Type II outbursts [PDF]
Binay Rai +5 more
openalex +1 more source

