Results 71 to 80 of about 43,788 (263)
PSR J1023+0038 is the first millisecond pulsar discovered to pulsate in the visible band; such a detection took place when the pulsar was surrounded by an accretion disk and also showed X-ray pulsations.
Ambrosino, F. +24 more
core +1 more source
Analytical Description of the Distributions of Primary and Secondary Cosmogenic Particles
In this work, we present an analytical description of the energy distributions of primary and secondary cosmogenic particles on Earth in terms of parameters having clear physical meaning. A modified power law is assumed for energy distributions, incorporating terms such as energy loss/decay, which are effective at low energies, and a source term, which
Shvetaank Tripathi +2 more
wiley +1 more source
The development of efficient and scalable catalysts for polyether amine (PEA) synthesis via reductive amination remains an enduring industrial challenge. In this study, bimetallic NiCu alloys supported on amorphous alumina were rationally designed for the amination of low‐molecular‐weight polyether (PPG‐230).
Hongyan Yu +9 more
wiley +1 more source
Multiwavelength Study of HESS J0632+057: New Insights into Pulsar–Disk Interaction
We present an analysis of new multiwavelength observations of the TeV gamma-ray binary HESS J0632+057, conducted using SALT, Swift, NuSTAR, and VERITAS in 2023–2024.
Jaegeun Park +61 more
doaj +1 more source
The nebula around pulsar B1853+01 in X-rays
We report on the results of a comprehensive analysis of X-ray observations with Chandra, XMM-Newton and NuSTAR of the pulsar wind nebula (PWN) associated with PSR B1853+01, located inside the W44 supernova remnant (SNR).
Zhang Xiying +3 more
doaj +1 more source
Detection of an X-ray Pulsation for the Gamma-ray Pulsar Centered in CTA 1
We report the detection of X-ray pulsations with a period of ~315.87 ms from the 2009 XMM-Newton observation for the radio-quiet gamma-ray pulsar, LAT PSR J0007+7303, centered in the supernova remnant CTA 1.
Abdo +17 more
core +1 more source
New Arabic Records From Cairo on Supernovae 1181 and 1006
ABSTRACT The remnant of the historical supernova SN 1181 is under discussion: While the previously suggested G130.7+3.1 (3C58) appears too old (3000–5000 year), the unusual star IRAS00500+6713 with a surrounding nebula (Pa‐30) has an expansion age not inconsistent with a SN Iax explosion in ad 1181 under the assumption that neither acceleration nor ...
J. G. Fischer +3 more
wiley +1 more source
Optical observations of PSR J2021+3651 in the Dragonfly Nebula with the GTC
PSR J2021+3651 is a 17 kyr old rotation powered pulsar detected in the radio, X-rays, and $\gamma$-rays. It powers a torus-like pulsar wind nebula with jets, dubbed the Dragonfly, which is very similar to that of the Vela pulsar.
Cabrera-Lavers, Antonio +9 more
core +1 more source
Discovery of an Energetic Pulsar Associated with SNR G76.9+1.0 [PDF]
We report the discovery of PSR J2022+3842, a 24 ms radio and X-ray pulsar in the supernova remnant G76.9+1.0, in observations with the Chandra X-ray telescope, the Robert C. Byrd Green Bank Radio Telescope, and the Rossi X-ray Timing Explorer (RXTE). The
Arzoumanian, Z. +5 more
core +3 more sources
Abstract CO2 methanation with Ni/Al2O3 catalysts is a key technology for converting CO2 emissions into sustainable methane. However, conventional impregnation synthesis often results in poor nickel dispersion and in the emission of gaseous NOx species.
Anderson F. C. Silva +2 more
wiley +1 more source

