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INTEGRAL Observations of Magnetars [PDF]
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT The INTEGRAL satellite has collected a large amount of data on magnetars in our Galaxy, spanning more than 20 years starting from 2003. The large data set obtained with the IBIS/ISGRI instrument at energies above 20 keV allows us to study both the properties and long‐term evolution of their persistent hard X‐ray emission and the population ...
Dominik Patryk Pacholski +3 more
wiley +5 more sources
Annual Review of Astronomy and Astrophysics, 2017 International audienceWhat is the origin of neutron star magnetic fields ? Although the fossil field hypothesis (i.e. the amplification of the neutron star progenitor field by flux conservation) would be the simplest mechanism, it seems unlikely to ...
Raynaud, Raphaël, Guilet, Jérôme
core +8 more sources
Monthly Notices of the Royal Astronomical Society, 2019 We consider the current observed ensemble of pulsing ultraluminous X-ray sources (PULXs). We show that all of their observed properties (luminosity, spin period, and spin-up rate) are consistent with emission from magnetic neutron stars with fields in ...
Jean-Pierre Lasota (7808069) +1 more
core +14 more sources
Wind braking of magnetars: To understand magnetars' multiwave radiation properties [PDF]
Astronomische Nachrichten, 2014 Magnetars are proposed to be peculiar neutron stars powered by their super-strong magnetic field. Observationally, anomalous X-ray pulsars and soft gamma-ray repeaters are believed to be magnetar candidates.
Tong, H., Xu, R. X.
core +3 more sources
Multipolar Electromagnetic Emission of Newborn Magnetars
The Astrophysical JournalIt is generally recognized that the electromagnetic multipolar emission from magnetars can be used to explain radiation from soft gamma repeaters or anomalous X-ray pulsars, but they have little impact on the spin-down of magnetars.
Yu Wang, Rahim Moradi, Liang Li
doaj +2 more sources
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
doaj +2 more sources
The Galactic Population of Magnetars: A Simulation-based Inference Study
The Astrophysical JournalPopulation synthesis modeling of the observed dynamical and physical properties of a population is a highly effective method for constraining the underlying birth parameters and evolutionary tracks.
M. Sautron +5 more
doaj +2 more sources
Numerical simulations of the tayler-spruit dynamo in proto-magnetars [PDF]
, 2023 International audienceThe Tayler–Spruit dynamo is one of the most promising mechanisms proposed to explain angular momentum transport during stellar evolution. Its development in proto-neutron stars spun-up by supernova fallback has also been put forward
Raynaud, Raphaël +11 more
core +1 more source
The Zoo of Isolated Neutron Stars
Universe, 2023 In this brief review, I summarize our basic knowledge about different types of isolated neutron stars. I discuss radio pulsars, central compact objects in supernova remnants, magnetars, nearby cooling neutron stars (also known as the magnificent seven ...
Sergei B. Popov
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R-Process with Magnetized Nuclei at Dynamo-Explosive Supernovae and Neutron Star Mergers
Universe, 2021 Nucleosynthesis at latge magnetic induction levels relevant to core-collapse supernovae and neutron star mergers is considered. For respective magnetic fields of a strength up to ten teratesla, atomic nuclei exhibit a linear magnetic response due to the ...
Vladimir N. Kondratyev
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