Results 31 to 40 of about 525 (178)
QED plasma and magnetars [PDF]
Journal of Cosmology and Astroparticle Physics, 2016 5 pages, v2: references added, formatting ...
Freytsis, Marat, Gralla, Samuel E.
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Solving the Mystery of Fast Radio Bursts: A Detective’s Approach
Universe, 2023 Fast radio bursts (FRBs) are still a mystery in contemporary astrophysics. Unlike many other astronomical objects whose basic physical mechanism is already identified and the research on which focuses mainly on refining details, FRBs are still largely ...
Bing Zhang
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, 2007 Thanks to INTEGRAL's long exposures of the Galactic Plane, the two brightest Soft Gamma-Ray Repeaters, SGR 1806-20 and SGR 1900+14, have been monitored and studied in detail for the first time at hard-X/soft-gamma rays. SGR 1806-20, lying close to the Galactic Centre, and being very active in the past two years, has provided a wealth of new INTEGRAL ...
Götz, D. +7 more
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THE McGILL MAGNETAR CATALOG [PDF]
The Astrophysical Journal Supplement Series, 2014 24 pages, 8 tables, 16 figures. Accepted for publication in The Astrophysical Journal Supplement Series.
Olausen, S. A., Kaspi, V. M.
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Searching for radio emission from radio quiet magnetars with MeerKAT
Astronomy & AstrophysicsContext. Magnetars are neutron stars that occupy the extreme end of the neutron star population, with magnetic field strengths greater than 1012 G.
Bause Marlon L. +3 more
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An overview of light ray deflection calculation by magnetars in nonlinear electrodynamics
Қарағанды университетінің хабаршысы. Физика сериясыDue to the lack of experimental confirmation of the effects of nonlinear electrodynamics (NED) of vacuum on the electromagnetic wave, it remains the most pressing issue. One of the most optimal media for studying these effects, occurring in astrophysics,
Н. Бейсен +7 more
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European Physical Journal C: Particles and FieldsThe initial spin periods of newborn magnetars are strongly associated with the origin of their strong magnetic fields, both of which can affect the electromagnetic radiation and gravitational waves (GWs) emitted at their birth. Combining the upper limit $
Yu-Long Yan +3 more
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UniverseRobust age measurements for isolated neutron stars (NSs) are not easily available. That is why the characteristic age τch=P/2P˙ is often used as a proxy. Here, P is the spin period of the NS and P˙ is the time derivative of P.
Rostislav D. Nikandrov, Sergei B. Popov
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XMM‐Newton Observations of the Peculiar Be X‐Ray Binary A0538‐66
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT A0538‐66 is a neutron star/Be x‐ray binary located in the Large Magellanic Cloud and, since its discovery in the 70s, it showed a peculiar behavior that makes it a unique object in the high‐mass x‐ray binaries scene: the extremely eccentric orbit (e=0.72$$ e=0.72 $$), the short spin period of the neutron star (P=69$$ P=69 $$ ms), the episodes ...
Michela Rigoselli +3 more
wiley +1 more source
Monthly Notices of the Royal Astronomical Society, 2019 8 pages, 1 figure, MNRAS ...
Andrew King, Jean-Pierre Lasota
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