Results 1 to 10 of about 418,649 (286)

X-Ray Binaries: A Potential Dominant Contributor to the Cosmic-Ray Spectral Knee Structure

The Astrophysical Journal
“PeVatrons” refer to astrophysical sources capable of accelerating particles to energies of ∼PeV and higher, potentially contributing to the cosmic-ray spectrum in the knee region.
Hua Yue, Jianli Zhang, Yuhai Ge, Lin Nie, Peipei Zhang, Wei Liu, Yiqing Guo, Hongbo Hu   +7 more
doaj   +1 more source

High-mass X-ray binaries as a star formation rate indicator in distant galaxies [PDF]

, 2003
H. J. Grimm, M. Gilfanov, R. Sunyaev
openalex   +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

Longterm properties of accretion discs in X-ray Binaries - III. A search for spin-superorbital correlation in SMC X-1 [PDF]

, 2018
Kristen C. Dage, W. I. Clarkson, P. A. Charles, S. Laycock, I. C. Shih   +4 more
openalex   +1 more source

IGR J19294+1816: a new Be-X-ray binary revealed through infrared spectroscopy [PDF]

, 2018
J. J. Rodes‐Roca, Guillermo Bernabeu, A. Magazzù, J. M. Torrejón, E. Solano   +4 more
openalex   +1 more source

Global Accretion Properties of Black Hole X-Ray Binaries: A Phenomenological Perspective [PDF]

, 2022
Arghajit Jana
openalex   +1 more source

Formation of twin compact stars in low-mass X-ray binaries [PDF]

S. Chanlaridis, D. Ohse, David Alvarez-Castillo, John Antoniadis, D. Blaschke, Victor I. Danchev, N. Langer, Devina Misra   +7 more
openalex   +1 more source

Long-term radio monitoring of the neutron star X-ray binary Swift J1858.6−0814

, 2022
Lauren Rhodes, R. P. Fender, S. Motta, J. van den Eijnden, D. R. Williams, Joe Bright, G. R. Sivakoff   +6 more
openalex   +1 more source

The Long-term Spin-down Trend of Ultraluminous X-Ray Pulsar M82 X-2

The Astrophysical Journal
The discovery in 2014 of the pulsation from the ultraluminous X-ray source (ULX) M82 X-2 has changed our view of ULXs. Because of the relatively short baseline over which pulsations have been detected so far, M82 X-2's spin state had been assumed to be ...
Jiren Liu
doaj   +1 more source

THE MAGNETOHYDRODYNAMICAL MODEL OF KILOHERTZ QUASI-PERIODIC OSCILLATIONS IN NEUTRON STAR LOW-MASS X-RAY BINARIES (II) [PDF]

, 2014
Chang-Sheng Shi, Shuang‐Nan Zhang, Xiang‐Dong Li   +2 more
openalex   +1 more source