Results 81 to 90 of about 525 (178)
Fast blue optical transients (FBOTs) are luminous, rapidly evolving events with blue spectra, possibly powered by newborn magnetars and linked to fast radio bursts (FRBs).
Shi-Jie Gao +7 more
doaj +1 more source
We explain the braking index n=2.19±0.03 of PSR J1846−0258 by incorporating the time evolution of its magnetic inclination angle and dipolar magnetic field. Based on observational timing data and the age of the associated supernova remnant (tSNR≈1.77kyr),
Biao-Peng Li +8 more
doaj +1 more source
IXPE detection of polarized X-rays from magnetars and photon mode conversion at QED vacuum resonance. [PDF]
Lai D.
europepmc +1 more source
Fast Radio Bursts as Sources of Ultra-High-Energy Cosmic Rays: A Multi-Messenger Review
Fast radio bursts (FRBs) are millisecond-duration radio transients of extragalactic origin, while ultra-high-energy cosmic rays (UHECRs; E≳1018 eV) remain among the most important unresolved problems in astroparticle physics.
Luiz Augusto Stuani Pereira
doaj +1 more source
Discovery of a radio emitting neutron star with an ultra-long spin period of 76 seconds. [PDF]
Caleb M +21 more
europepmc +1 more source
A commentary of "Consistency radio bursts in the Milky Way": 10 remarkable discoveries from 2020 in Nature. [PDF]
Li D.
europepmc +1 more source
A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism. [PDF]
Zhu W +36 more
europepmc +1 more source
Internal constitution of the outer crust of non-accreted neutron stars and magnetars
Context. Determining the internal constitution of the outer crust of magnetars is important for interpreting several of their astrophysical manifestations. In particular, the crustal composition is a key input for simulations of r-process nucleosynthesis
Servais J., Chamel N.
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Life Unknown: Preliminary Scheme for a Magnetotrophic Organism. [PDF]
Schulze-Makuch D, Irwin LN.
europepmc +1 more source
Hydrogen-poor Superluminous Supernovae with Bumpy Light Curves Powered by Precessing Magnetars
Recent observations and statistical studies have revealed that a significant fraction of hydrogen-poor superluminous supernovae (SLSNe-I) exhibit light curves that deviate from the smooth evolution predicted by the magnetar-powered model, instead showing
Biao Zhang +3 more
doaj +1 more source

