Results 51 to 60 of about 93,185 (169)
Magnetic Fields in Supernova Remnants
Parkes 2 7 and 5 0 GHz polarization maps have been combined to obtain distributions of magnetic field, Faraday rotation and depolarization for 20 supernova remnants.
DK Milne, John R Dickel
core +1 more source
Suprathermal Electron Acceleration Comparison of the Venusian and Terrestrial Bow Shocks
Abstract We study suprathermal electron acceleration at the Venusian bow shock using the Parker Solar Probe gravity assists and the Venus Express spacecraft mission. The acceleration is classified by measuring the maximum energy and the power‐law spectral slope (index) of the electron phase space density immediately downstream of the shocks for ...
M. Lindberg +4 more
wiley +1 more source
MeerKAT 1.3 GHz Observations of Supernova Remnants
We present full Stokes MeerKAT L -band (856–1712 MHz) observations of 36 high-latitude supernova remnants (SNRs). Sensitive, high-dynamic-range images show a wealth of structure. G15.1−1.6 appears to be a H ii region rather than an SNR.
W. D. Cotton +5 more
doaj +1 more source
Abstract Recent works suggest there are periods when the Sun encountered massive interstellar cold clouds which compressed the heliosphere to within Earth's orbit, exposing Earth to interstellar galactic cosmic rays and energetic particles of heliospheric origin.
Anna Nica +4 more
wiley +1 more source
Three-dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tycho's Supernova Remnant
While various methods have been proposed to disentangle the progenitor system for Type Ia supernovae, their origin is still unclear. A circumstellar environment is key to distinguishing between the double-degenerate and single-degenerate (SD) scenarios ...
Hiroyuki Uchida +5 more
doaj +1 more source
ABSTRACT Background Despite the end of the pandemic phase, patients with hematological malignancies (HMs) remain vulnerable to severe COVID‐19 infection and mortality. Prophylaxis strategies, including vaccination and monoclonal antibodies (mAbs) like AZD7442, are crucial for protection.
Mubarak Al‐Mansour +8 more
wiley +1 more source
In situ x‐ray transmission imaging and monochromatic small angle x‐ray scattering (SAXS) measurements of Au precursor solution establish that precise tuning of incident photon energy controls not only the radiolytic yield but the entire hierarchical aggregation trajectory, offering a sophisticated blueprint for the rational design of functional ...
Akinobu Yamaguchi +5 more
wiley +1 more source
Searching for Supernova Remnants
The UKST/AAO Galactic Plane Hα Survey has the potential to discover many new objects not visible on red plates taken in past surveys. Recent radio surveys have identified large numbers of new supernova remnants, very few of which have been optically ...
W. J. Zealey, A. Walker
core +1 more source
Detection of Gamma-Ray Emission from Supernova Remnant G156.2+5.7
G156.2+5.7 is a supernova remnant (SNR) characterized by strong X-ray emission and low radio surface brightness. To investigate its high-energy gamma-ray emission, we analyzed more than 17 yr of Fermi Large Area Telescope data.
Yangxuan Diao, Siming Liu, Xi Liu
doaj +1 more source
Supernova Remnants in Gamma Rays
In the 1960s, the remnants of supernova explosions (SNRs) were indicated as a possible source of galactic cosmic rays through the Diffusive Shock Acceleration (DSA) mechanism.
Andrea Giuliani, Martina Cardillo
doaj +1 more source

