The Magellanic Clouds host a large population of high-mass X-ray binary (HMXB) systems, but although the Large Cloud (LMC) is an order magnitude more massive than Small Cloud, significantly fewer HMXBs are known. We conducted search for new in XMM-Newton observations, which we performed to investigate supernova remnant candidates supergiant shells LMC5 and LMC7. three observed fields located re...

X Persei is a persistent low-luminosity X-ray pulsar of period $\sim$835 s in Be binary system. The field strength at the neutron star surface not known precisely, but indirect signs indicate magnetic above $10^{13}$ G, which makes object one most magnetized pulsars. Here we present results observations performed with Imaging Polarimetry Explorer (IXPE). polarization signal was found to be stro...

Introduction: To date, gold nanoparticles (GNPs) have been demonstrated to have great potential as contrast agent for CT imaging and therapeutics. This study was designed to evaluate any effect on X-ray attenuation that might result from using GNPs with a variety of size, surface chemistries and shapes.   Materials and Methods: Spherical GNPs and gold nanorod...

Background: People occasionally undergo medical diagnostic X-ray examinations and expose their red blood cells to radiation. Radiation that is generated from medical diagnostic X-ray machines is widely used in medical diagnoses. One of the important parameters is kilo-voltage (kV) that is applied across the X-ray tube in medical diagnostic X-ray machines. Kilo-voltage influences the radiation d...

We present an analysis of the optical properties three Ultra Luminous X-ray (ULX) sources identified in NGC 925. use Integral field unit data from George Mitchel spectrograph context Metal-THINGS survey. The for ULX-1 and ULX-3 are presented, while spaxel associated with ULX-2 had a low S/N, which prevented its analysis. also report kinematics dimensions nebula each ULX using ancillary PUMA Fab...