Magnetars are young and highly magnetized neutron stars that display a wide array of X-ray
activity including short bursts, large outbursts, giant flares, and quasi-periodic oscillations …

Magnetars are the strongest magnets in the present universe and the combination of
extreme magnetic field, gravity and density makes them unique laboratories to probe current …

Observations of magnetars and some of the high magnetic field pulsars have shown that
their thermal luminosity is systematically higher than that of classical radio-pulsars, thus …

The strong magnetic field of neutron stars is intimately coupled to the observed temperature
and spectral properties, as well as to the observed timing properties (distribution of spin …

Magnetospheres of neutron stars are anchored in the rigid crust and can be twisted by
sudden crustal motions (" starquakes"). The twisted magnetosphere does not remain static …

We report on the lowest-frequency detection to date of three bursts from the fast radio burst
FRB 180916. J0158+ 65, observed at 328 MHz with the Sardinia Radio Telescope (SRT) …

Magnetars are neutron stars in which a strong magnetic field is the main energy source.
About two dozens of magnetars, plus several candidates, are currently known in our Galaxy …

We study the conditions for the adiabatic resonant conversion of the cold dark matter (CDM)
axions into photons in the astrophysically sourced strong magnetic fields such as those in …

Neutron stars are compact and dense celestial objects that offer the unique opportunity to
explore matter and its interactions under conditions that cannot be reproduced elsewhere in …

Ray tracing plays a vital role in black hole imaging, modeling the emission mechanisms of
pulsars, and deriving signatures from physics beyond the Standard Model. In this work we …