Results 91 to 100 of about 525 (178)
, 2007 Slow dissipation of non-potential magnetic fields in the magnetosphere of the magnetar is assumed to accelerate particles to hundreds MeV along the magnetic field lines. We consider interaction of fast particles with the surface of the magnetar. We argue that the collisionless dissipation does not work in the atmosphere of the neutron star because the ...
Lyubarsky, Yury, Eichler, David
openaire +2 more sources
A Unified Volumetric Rate–Energy Relation from Magnetar Radio Bursts to Fast Radio Bursts
The Astrophysical JournalFast radio bursts (FRBs) are millisecond radio pulses with extremely high bright temperature. Their physical origin is still a mystery. The discovery of FRB 20020428 supports the idea that at least a portion of FRBs is generated by magnetars.
Hao-Tian Lan, Shuang-Xi Yi, Fa-Yin Wang
doaj +1 more source
Investigating the Recursive Short X-Ray Burst Behavior of Magnetars through Crustal Interactions
The Astrophysical JournalEnergetic bursts from strongly magnetized neutron stars, known as magnetars, are typically detected in clusters. Once an active episode begins, anywhere from a few to thousands of hard X-ray bursts can occur over durations ranging from days to months ...
Özge Keskin +2 more
doaj +1 more source
Physics of Neutron Star Crusts
Living Reviews in Relativity, 2008 The physics of neutron star crusts is vast, involving many different research fields, from nuclear and condensed matter physics to general relativity.
Chamel Nicolas, Haensel Pawel
doaj
China's 'sky eye': exploring the universe by measuring faint cosmic radio signals. [PDF]
Natl Sci Rev, 2023 Zhao W.
europepmc +1 more source
The Astrophysical Journal LettersIn addition to being the most magnetic objects in the known Universe, magnetars are the only objects observed to generate fast-radio-burst-like emissions. The formation mechanism of magnetars is still highly debated and may potentially be probed with the
Hao Ding +5 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
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
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