Results 141 to 150 of about 525 (178)
Bridging the gap: from massive stars to supernovae. [PDF]
Philos Trans A Math Phys Eng Sci, 2017 Maund JR +3 more
europepmc +1 more source
Management succinate release through SDHA by G protein-coupled receptor 91 signal, TRAP1, and SIRT3 regulation in lung cancer cells by NAR nanoparticles. [PDF]
J Genet Eng BiotechnolRagab EM +3 more
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Extended main sequences in star clusters. [PDF]
Fundam ResLi C, Milone AP, Sun W, de Grijs R.
europepmc +1 more source
Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]
Space Sci RevLiu YH +14 more
europepmc +1 more source
Brazilian 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, Mereghetti Sandro
exaly +3 more sources
Pulse frequency fluctuations of magnetars [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 18 pages, 1 table, 4 figures, accepted for publication in ...
Abdulhadi Baykal +2 more
exaly +5 more sources
The early evolution of magnetar rotation – I. Slowly rotating ‘normal’ magnetars
Monthly Notices of the Royal Astronomical Society, 2022 ABSTRACT In the seconds following their formation in core-collapse supernovae, ‘proto’-magnetars drive neutrino-heated magnetocentrifugal winds. Using a suite of two-dimensional axisymmetric magnetohydrodynamic simulations, we show that relatively slowly rotating magnetars with initial spin periods of P⋆0 = 50–500 ms spin down rapidly ...
Matthew S B Coleman +2 more
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Wind braking of magnetars: To understand magnetars' multiwave radiation properties [PDF]
Astronomische Nachrichten, 2014 AbstractMagnetars 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. While more and more multiwave observations of magnetars are available, we see unfortunately an accumulation of failed predictions of the ...
Tong, H., Xu, R. X.
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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
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