China's 'sky eye': exploring the universe by measuring faint cosmic radio signals. [PDF]
Natl Sci Rev, 2023 Zhao W.
europepmc +1 more source
Toward Understanding the Origin of Swift Gamma-Ray Bursts Driven by Magnetars
The Astrophysical JournalIn this paper, we analyze a sample of Swift gamma-ray bursts (GRBs) with extended emissions in γ -rays and/or X-ray plateaus that may be driven by magnetars.
C. T. Hao +9 more
doaj +1 more source
Modeling Isolated Magnetar Spin-down Evolution and Implications for Long-period Radio Transients
The Astrophysical JournalLong-period radio transients (LPTs) are a new class of radio sources characterized by long spin periods ( P _spin > 10 ^3 s) and highly variable radio emission. While known magnetars are relatively young ( τ 10 ^3 s.
Jon Kwong, Kaya Mori
doaj +1 more source
Repeating fast radio burst 20201124A originates from a magnetar/Be star binary. [PDF]
Nat Commun, 2022 Wang FY, Zhang GQ, Dai ZG, Cheng KS.
europepmc +1 more source
Electromagnetic wave transparency of X mode in strongly magnetized plasma. [PDF]
Sci Rep, 2021 Mandal D, Vashistha A, Das A.
europepmc +1 more source
Discovery of Evolution of the Temporal Features of X-Ray Bursts from SGR J1935+2154
The Astrophysical JournalSGR J1935+2154 has undergone eight active episodes since its discovery in 2014. In this study, our focus is on the evolution of the temporal characteristics including burst duration, minimum variation timescale (MVT), and waiting time across these active
Shuo Xiao +9 more
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Polarized X-Rays Detected from the Anomalous X-Ray Pulsar 1E 2259+586
The Astrophysical JournalAnomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are believed to be associated with magnetars, which have extremely strong magnetic fields.
Han-Long Peng +7 more
doaj +1 more source
Neutrino communication, intergalactic transit, and Astrobiology. [PDF]
Bioinformation, 2022 Shapshak P.
europepmc +1 more source
Hyperactive Magnetar Eruptions: Giant Flares, Baryon Ejections, and Fast Radio Bursts
The Astrophysical Journal LettersYoung neutron stars born with magnetic fields B ≳ 10 ^16 G become hyperactive as the field inside the star evolves through ambipolar diffusion on a timescale ∼10 ^9 s.
Ashley Bransgrove +2 more
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Gravitational waves from magnetars
International Journal of Modern Physics DWe study the emission of gravitational waves produced by the magnetosphere of magnetars. We argue that several features in the spectrum could facilitate the identification of that source. In addition, in cases of extremely large magnetic fields we demonstrate that this emission can contribute to the deviation of the braking index from 3, which is the ...
openaire +2 more sources