高速電波バースト(FRB)は、その起源が謎に包まれているものの、電波観測だけでなく、X線、ガンマ線、ニュートリノ、重力波など、様々な波長やメッセンジャーで対応天体の探索が進められている。
While the exact nature of fast radio bursts (FRBs) remains elusive, the association of FRB 20200428D with a Galactic magnetar suggests a possible origin. This paper explores various theoretical models and observational evidence for multi-wavelength and multi-messenger counterparts to FRBs, highlighting the challenges and future prospects in understanding these enigmatic events.
The rotational mass of anisotropic neutron stars is significantly impacted by the Rastall gravity parameter and the anisotropic strength, with the anisotropic strength being the dominant factor. The mass constraints of observed neutron stars, including the heaviest known, can be satisfied by the model with strong anisotropic strength.
The presence of mirror dark matter can explain the unusual mass and radius measurements of compact objects like XTE J1814-338, which challenge conventional neutron star models.
The discovery of a 5.33 millisecond pulsar, PSR J1750-3116A, likely associated with the globular cluster Terzan 6, which has an exceptionally high stellar encounter rate suggesting it should harbor dozens of pulsars.
Accreting neutron stars in binary-driven hypernovae can reach the critical mass for gravitational collapse into a black hole, with the occurrence time depending on the initial angular momentum and accretion efficiency.
Scintillation analyses of eight canonical pulsars over 2.5 years reveal new insights into the structure and evolution of the interstellar medium along their lines of sight.
The BlackCAT CubeSat mission is expected to detect a mean of 42 long-duration gamma-ray bursts per year, with 6.7% to 10% of these at redshifts z > 3.5.
Pulsars can power extended, linear X-ray filaments through the escape of ultra-relativistic electrons and positrons from their bow shocks, which then radiate synchrotron emission along the ambient magnetic field lines.
TIC 290061484 is a triply eclipsing quadruple star system with the shortest known outer period of only 24.5 days, significantly shorter than the previous record holder.