Results 161 to 170 of about 8,336 (234)

Radio Observation of the Pulsar Wind Nebula in Supernova Remnant G11.2−0.3

open access: yesThe Astrophysical Journal
Pulsar wind nebulae (PWNe) are important sources for understanding galactic high-energy processes, but it is controversial until now how high-energy particles in PWNe are accelerated and transported. Lacking radio counterparts of X-ray PWNe (the proposed
Yu Zhang   +4 more
doaj   +1 more source

Kilonovae. [PDF]

open access: yesLiving Rev Relativ, 2020
Metzger BD.
europepmc   +1 more source

Multiband Nonthermal Radiative Study of PeVatron Candidate Pulsar Wind Nebula HESS J1849-000

open access: yesThe Astrophysical Journal
Pulsar wind nebula HESS J1849-000 is one of the sources that may emit PeV γ -ray photons based on the recent measurement by the Tibet Air Shower Array and the Large High Altitude Air Shower Observatory.
Bo-Tao Zhu, Fang-Wu Lu, Li Zhang
doaj   +1 more source

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