Results 161 to 170 of about 3,165 (200)

Grand unification of neutron stars. [PDF]

open access: yesProc Natl Acad Sci U S A, 2010
Kaspi VM.
europepmc   +1 more source

Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Nakamura R   +24 more
europepmc   +1 more source

When the Milky Way hosted a quasar

open access: yes, 2022
Marin F   +103 more
europepmc   +1 more source

Pulse frequency fluctuations of magnetars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
Using RXTE, Chandra, XMM-Newton and Swift observations, we construct the power spectra and torque noise strengths of magnetars for the first time. For some of the sources, on time-scales of months to years, we measure strong red noise that might be a ...
Abdulhadi Baykal   +2 more
exaly   +6 more sources

Pulsars and Magnetars [PDF]

open access: yesBrazilian Journal of Physics, 2013
The high-energy sources known as anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs) are well explained as magnetars: isolated neutron stars powered by their own magnetic energy. After explaining why it is generally believed that the traditional energy sources at work in other neutron stars (accretion, rotation, residual heat) cannot ...
Sandro Mereghetti
exaly   +3 more sources

An observational argument against accretion in magnetars

open access: yesAstronomy and Astrophysics, 2020
© ESO 2020. The phenomenology of anomalous X-ray pulsars is usually interpreted within the paradigm of very highly magnetized neutron stars, also known as magnetars. According to this paradigm, the persistent emission of anomalous X-ray pulsars (AXPs) is
Víctor Doroshenko   +2 more
exaly   +1 more source

Observations of Magnetars

AIP Conference Proceedings, 2008
The salient properties of magnetars are summarized here with an emphasis on recent developments in the field since 2005. In particular, I discuss observations of the giant flares, bursts from Anomalous X‐ray Pulsars (AXPs), transient emission from AXPs, multi‐wavelength observations of magnetars, glitch activity in AXPs, magnetar energy spectra, and ...
Peter M. Woods   +4 more
openaire   +1 more source

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