Results 61 to 70 of about 53,953 (346)

Three Additional Quiescent Low-Mass X-Ray Binary Candidates in 47 Tucanae [PDF]

, 2004
We identify through their X-ray spectra one certain (W37) and two probable (W17 and X4) quiescent low-mass X-ray binaries (qLMXBs) containing neutron stars in a long Chandra X-ray exposure of the globular cluster 47 Tucanae, in addition to the two ...
C. Heinke, C. Heinke, J. Grindlay, P. Edmonds   +3 more
semanticscholar   +1 more source

Low-Magnetic-Field Neutron Stars in X-ray Binaries

, 2023
In this chapter we give an overview of the properties of X-ray binary systems containing a weakly magnetized neutron star. These are old (Giga-years life-time) semi-detached binary systems containing a neutron star with a relatively weak magnetic field (less than $\sim 10^{10}$ Gauss) and a low-mass (less than $1 M_\odot$) companion star orbiting ...
Di Salvo, Tiziana, Papitto, Alessandro, Marino, Alessio, Iaria, Rosario, Burderi, Luciano   +4 more
openaire   +2 more sources

Z‐Scheme Water Splitting Systems Based on Solid‐State Electron Conductors

Advanced Functional Materials, EarlyView.
This review examines the latest advances in Z‐scheme overall water splitting (OWS) systems for solar hydrogen production. These systems consist of suspended or immobilized hydrogen evolution photocatalysts (HEPs) and oxygen evolution photocatalysts (OEPs).
Chen Gu, Takashi Hisatomi, Tsuyoshi Takata, Kazunari Domen   +3 more
wiley   +1 more source

Discovery of a New Phase-transient Cyclotron Line in A0535+26: Constraints on the Accretion Geometry

The Astrophysical Journal
In 2020 November, A0535+26 underwent one of its brightest outbursts, reaching nearly 12 Crab in X-ray flux. Observed by Insight-HXMT, NuSTAR, NICER, and AstroSat, this event provided valuable insights into Be/X-ray binaries.
Ashwin Devaraj, Biswajit Paul, Varun Bhalerao, Dipanjan Mukherjee   +3 more
doaj   +1 more source

Physics of Binary Star Evolution -- from Stars to X-ray Binaries and Gravitational Wave Sources [PDF]

, 2023
Thomas M. Tauris, E. P. J. van den Heuvel   +1 more
openalex   +1 more source

The globular cluster mass/low mass X-ray binary correlation: implications for kick velocity distributions from supernovae [PDF]

, 2006
Optical and X-ray studies of six nearby galaxies show that the probability a globular cluster will be an X-ray source is consistent with being linearly proportional to its mass.
M. Smits, T. Maccarone, T. Maccarone, A. Kundu, S. Zepf   +4 more
semanticscholar   +1 more source

Positive‐Tone Nanolithography of Antimony Trisulfide with Femtosecond Laser Wet‐Etching

Advanced Functional Materials, EarlyView.
A butyldithiocarbamic acid (BDCA) etchant is used to fabricate various micro‐ and nanoscale structures on amorphous antimony trisulfide (a‐Sb2S3) thin film via femtosecond laser etching. Numerical analysis and experimental results elucidate the patterning mechanism on gold (reflective) and quartz (transmissive) substrates.
Abhrodeep Dey, Uwe Hübner, Albane Benardais, Xiaofei Wu, Andrea Dellith, Jan Dellith, Torsten Wieduwilt, Henrik Schneidewind, Markus A Schmidt, Virginie Nazabal, Volker Deckert, Jer‐Shing Huang, Wei Wang   +12 more
wiley   +1 more source

Orbital Phase-resolved Analysis of X-Ray and Gamma-Ray Observations of the High-mass Gamma-Ray Binary 4FGL J1405.1−6119

The Astrophysical Journal
We present the results of multiwavelength observations of the high-mass gamma-ray binary (HMGB) 4FGL J1405.1−6119. A pair of joint XMM-Newton and NuSTAR observations taken in 2019 (sampling the gamma-ray maximum and X-ray maximum) characterize the ...
Alexander Lange, Robin H.D. Corbet, Joel B. Coley, Guillaume Dubus, Jeremy Hare, Nazma Islam, Jonathan Barnes   +6 more
doaj   +1 more source

Modelling the expected very high energy gamma-ray emission from accreting neutron stars in X-ray binaries [PDF]

, 2023
L. Ducci, P. Romano, S. Vercellone, A. Santangelo   +3 more
openalex   +1 more source

Spectroscopic observations of the candidate sgB(e)/X-ray binary CI Camelopardalis [PDF]

, 2002
We present a compilation of spectroscopic observations of the sgB(e) star CI Cam, the optical counterpart of XTE J0421+560. This includes data from before, during, and after its 1998 outburst, with quantitative results spanning 37 years. The object shows
R. Hynes, J. Clark, E. Barsukova, P. Callanan, P. Charles, A. Cameron, S. Fabrika, M. Garcia, C. Haswell, K. Horne, A. Miroshnichenko, I. Negueruela, P. Reig, W. Welsh, D. University, U. London, S. A. Observatory, University College Cork, S. University, Harvard-Smithsonian Cfa, T. O. University, U. Toledo, P. Observatory, O. Strasbourg, F. Crete, San Diego State University   +25 more
semanticscholar   +1 more source