Long-term Study of the 2020 Magnetar-like Outburst of the Young Pulsar PSR J1846-0258 in Kes 75
Magnetar-like activity has been observed in a large variety of neutron stars. PSR J1846−0258 is a young 327 ms radio-quiet pulsar with a large rotational power (∼8 × 10 ^36 erg s ^−1 ), and resides at the center of the supernova remnant Kes 75. It is one
R. Sathyaprakash +16 more
doaj +1 more source
Electromagnetic counterparts to massive black-hole mergers. [PDF]
Bogdanović T, Miller MC, Blecha L.
europepmc +1 more source
Model Spectra of Rotation Powered Pulsars in the INTEGRAL Range
The energy range of IBIS is a promising ground for testing mutual relations of distinct components expected in the spectra of high-energy radiation from rotation powered pulsars. According to some polar-cap models two such components - due to curvature and synchrotron emission - may contribute comparable amounts of power between 15 keV and 10 MeV ...
Dyks, J., Rudak, B., Bulik, T.
openaire +2 more sources
Magnetic Field Geometry of the Gamma-Ray Binary PSR B1259–63 Revealed via X-Ray Polarization
Some X-ray binaries containing an energetic pulsar in orbit around a normal star accelerate particles to high energies in the shock cone formed where the pulsar and stellar winds collide.
Philip Kaaret +8 more
doaj +1 more source
Astronomia ex machina: a history, primer and outlook on neural networks in astronomy. [PDF]
Smith MJ, Geach JE.
europepmc +1 more source
Emission From Rotation-Powered Pulsars: Is It All Relative?
10 pages, 6 figures, invited talk at 22nd Texas Symposium on Relativistic Astrophysics, Dec. 2004 (TSRA04-0040)
openaire +2 more sources
From Feast to Famine: A Systematic Study of Accretion onto Oblique Pulsars with 3D GRMHD Simulations
Disk-fed accretion onto neutron stars can power a wide range of astrophysical sources ranging from X-ray binaries, to accretion-powered millisecond pulsars, ultraluminous X-ray sources, and gamma-ray bursts.
Ariadna Murguia-Berthier +3 more
doaj +1 more source
Proper motion, spectra, and timing of PSR J1813-1749 using <i>Chandra</i> and <i>NICER</i>. [PDF]
Ho WCG +9 more
europepmc +1 more source
We analyzed X-ray data from Chandra, XMM-Newton, NICER, and NuSTAR to characterize the properties of the pulsar PSR J1838−0655 and its pulsar wind nebula (PWN) associated with HESS J1837−069.
Minseo Park +3 more
doaj +1 more source
Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and <i>γ</i>-Ray Bursts. [PDF]
Ruiz M, Shapiro SL, Tsokaros A.
europepmc +1 more source

