Article
Physics, Applied
Sanjay Chandra Andola, Ashutosh Chandrajeet Jaiswar, Trilok Chand Kaushik, Keshaw Datt Joshi
Summary: This report presents a comparative study on the properties of x-rays from X-pinches made of two groups of metallic wires. The study found that the Cu group requires a higher current to compress the plasma compared to the W group X-pinches. Additionally, a significant improvement in x-ray quality was observed in wires with a few micron thick dielectric coating. These findings are important for the development of a small capacitive X-pinch system suitable for high-energy density physics research.
JOURNAL OF PHYSICS D-APPLIED PHYSICS
(2022)
Article
Materials Science, Multidisciplinary
Milenko Vescovi, Felipe Veloso, Julio Valenzuela, Mario Favre
Summary: This paper presents a characterization of Cu X-pinches experiments driven at current rates around 1kA/ns. Two bursts of X-rays associated with hot-spot formation and electron beam-target mechanism are identified. The first burst is consistently correlated with the central hot-spot, while the second burst is associated with the electron beam-target mechanism.
RESULTS IN PHYSICS
(2021)
Article
Chemistry, Multidisciplinary
Alexandros Skoulakis, Evaggelos Kaselouris, Antonis Kavroulakis, Christos Karvounis, Ioannis Fitilis, John Chatzakis, Vasilis Dimitriou, Nektarios A. Papadogiannis, Michael Tatarakis
Summary: An X-pinch scheme of a low-current generator is characterized as a potential efficient source of soft X-rays, with the X-pinch target consisting of wires made from tungsten or gold-plated tungsten loaded at different angles. Time-resolved measurements showed different X-ray yields for different wire angles. The X-pinch was also found to be ideal for X-ray radiography applications.
APPLIED SCIENCES-BASEL
(2021)
Article
Physics, Applied
I. N. Tilikin, T. A. Shelkovenko, S. A. Pikuz, A. V. Oginov, A. R. Mingaleev, V. M. Romanova, A. E. Ter-Oganesyan
Summary: The study presents the results of radiation produced by the electrical explosion of a 4 μm thick Al foil with an artificial periodic structure of periodic holes. The experiments were conducted using a high-current generator and recorded using pinhole cameras and a microchannel plate camera. The results show that the application of an artificial periodic structure to the foil leads to a more uniform radiation distribution along the entire length and width of the foil. This uniform radiation can be used for imaging test objects or plasma objects like exploded wires.
JOURNAL OF APPLIED PHYSICS
(2023)
Article
Astronomy & Astrophysics
Pinaki Roy, Aru Beri, Sudip Bhattacharyya
Summary: Results from the study of 12 thermonuclear X-ray bursts in six AstroSat observations of a neutron star X-ray binary, 4U 1636 - 536, revealed strong evidence of thermonuclear flame spreading and latitude-dependent flame speeds, possibly influenced by the Coriolis force. The observations also indicated that the distance to the source estimated using photospheric radius expansion bursts is consistent with the known value of approximately 6 kpc.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
S. Vladutescu-Zopp, V. Biffi, K. Dolag
Summary: X-ray observations of galaxies have shown that X-ray bright point sources known as X-ray binaries contribute significantly to the diffuse X-ray emission of galaxies. This study provides a numerical framework to study the populations of X-ray binaries using hydrodynamical cosmological simulations. The numerical simulations reproduce observed scaling relations between X-ray luminosity and stellar mass, as well as between X-ray luminosity and star-formation rate. The modeling approach remains consistent with observations and holds great value for future investigations of galactic X-ray spectra.
ASTRONOMY & ASTROPHYSICS
(2023)
Article
Astronomy & Astrophysics
H. Stiele, A. K. H. Kong
Summary: We investigated the evolution of quasi-periodic oscillations (QPOs) and noise components using power-density spectra in five snapshots of NICER observations of the black hole transient GX 339-4 during its transition from the hard state to the soft state. We found a strong correlation between the hardness ratio and the type of QPO observed, suggesting a connection between the accretion geometry and spectral properties. We also observed that the type-B QPO undergoes a decoherence process during the transition between different states.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Ryan T. Urquhart, Roberto Soria, Rosanne Di Stefano, Kaiming Cui, Paolo Esposito, Gian Luca Israel, Sammarth Kumar, Sara Motta, Fabio Pintore, Giacomo Riva
Summary: This study investigates the unusual time variability of an ultraluminous X-ray source in M 101, identifying its bimodal behavior, fast outburst evolution, and the presence of strong quasi-periodic oscillations. These findings are significant for understanding the evolution and properties of similar celestial bodies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Dmitry Kolesnikov, Nikolai Shakura, Konstantin Postnov
Summary: Researchers found that the pulsation frequency and X-ray flux of Her X-1 show periodic variations, which can be explained by the free precession of a triaxial neutron star and mass readjustment.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
G. Q. Ding, T. T. Chen, J. L. Qu
Summary: The study systematically searches for hard X-ray tails in the X-ray spectra of Scorpius X-1 from 1996 to 2012, finding their presence is not confined to a specific position on the hardness-intensity diagram. The analysis suggests that the hard X-ray tail becomes harder and its flux decreases as the source transitions from the horizontal branch to the flaring branch on the diagram.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
D. R. A. Williams, S. E. Motta, R. Fender, J. C. A. Miller-Jones, J. Neilsen, J. R. Allison, J. Bright, I Heywood, P. F. L. Jacob, L. Rhodes, E. Tremou, P. A. Woudt, J. van den Eijnden, F. Carotenuto, D. A. Green, D. Titterington, A. J. van der Horst, P. Saikia
Summary: This study presents radio and X-ray observations of the candidate Black Hole X-ray Binary EXO 1846-031 during its 2019 outburst. Analysis of the data reveals the characteristic features of BHXB outbursts, and provides estimates of the energy of the radio flares and the time of return to "quiescence". Comparing the radio and X-ray data, the study also determines the position of EXO 1846-031 in the radio:X-ray plane during its "hard" state.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
E. Bozzo, C. Ferrigno, L. Oskinova, L. Ducci
Summary: 3A 1954+319 is a rare high-mass X-ray binary consisting of a neutron star and a red supergiant donor. The analysis of observational data reveals that the neutron star in this system possesses a magnetar-like magnetic field strength. This finding is significant for studying the accretion process of stars.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
D. J. Walton, A. D. A. Mackenzie, H. Gully, N. R. Patel, T. P. Roberts, H. P. Earnshaw, S. Mateos
Summary: The study presents a new catalogue of ULX candidates based on recent data releases from three X-ray observatories, identifying new extreme ULX candidate NGC3044 ULX1. The catalogue includes 1843 ULX candidates associated with 951 host galaxies and is expected to be a valuable resource for future observations of ULXs.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Physics, Applied
V Senthilkumaran, D. Bailie, K. Behm, J. Warwick, G. M. Samarin, A. Maksimchuk, J. Nees, A. G. R. Thomas, G. Sarri, K. Krushelnick, A. E. Hussein
Summary: This study focuses on the generation and propagation of focused gamma beams using laser wakefield accelerator technology. Experimental results and Monte Carlo simulations demonstrate the capacity of this technique and its potential applications in medical imaging and laboratory astrophysics experiments.
APPLIED PHYSICS LETTERS
(2022)
Article
Astronomy & Astrophysics
V Sguera, L. Sidoli, A. J. Bird, N. La Palombara
Summary: We present new results from INTEGRAL and Swift observations of the poorly studied and unidentified X-ray source XTE J1906+090. A bright hard X-ray outburst has been detected, as well as consistent low X-ray luminosity values. Based on our findings, we propose that XTE J1906+090 belongs to the small and rare group of persistent low-luminosity Be X-ray binaries.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)