Results 21 to 30 of about 125,993 (129)
The Thousand-Pulsar-Array programme on MeerKAT - X. Scintillation arcs of 107 pulsars [PDF]
We present the detection of 107 pulsars with interstellar scintillation arcs at 856–1712 MHz, observed with the MeerKAT Thousand Pulsar Array Programme.
R. Main+11 more
semanticscholar +1 more source
Fermi bubbles as sources of cosmic rays above 1 PeV
Fermi bubbles are giant gamma-ray structures extended north and south of the Galactic center with characteristic sizes of the order of 10 kpc discovered by the Fermi Large Area Telescope.
Chernyshov Dmitry+3 more
doaj +2 more sources
The nearest neutron star candidate in a binary revealed by optical time-domain surveys [PDF]
The near-Earth (within ∼100 pc) supernova explosions in the past several million years can cause the global deposition of radioactive elements (e.g., ^60Fe) on Earth. The remnants of such supernovae are too old to be easily identified. It is therefore of
Ling-Lin Zheng+21 more
semanticscholar +1 more source
Magnetic Imprisonment of Dusty Pinballs by a Supernova Remnant [PDF]
Motivated by recent measurements of deposits of 60Fe on the ocean floor and the lunar surface, we model the transport of dust grains containing 60Fe from a near-Earth (i.e., within 100 pc) supernova (SN).
Brian J. Fry, B. Fields, A. Ellis
semanticscholar +1 more source
The MicroBooNE continuous readout stream for detection of supernova neutrinos [PDF]
Since the original detection of core-collapse supernova neutrinos in 1987, all large neutrino experiments seek to detect the neutrinos from the next nearby supernova.
J. I. Crespo-Anadón
semanticscholar +1 more source
Gravitational Lensing of Supernova Neutrinos [PDF]
The black hole at the center of the galaxy is a powerful lens for supernova neutrinos. In the very special circumstance of a supernova near the extended line of sight from Earth to the galactic center, lensing could dramatically enhance the neutrino flux
Mena, Olga, Mocioiu, Irina, Quigg, Chris
core +3 more sources
Phosphorus in the Young Supernova Remnant Cassiopeia A [PDF]
We Are Stardust Most of the universe's chemical elements were produced in stars, with the heaviest elements being produced when stars explode. Barlow et al. (p. 1343) used the Herschel Space Observatory to obtain submillimeter spectra of the Crab Nebula,
B. Koo+4 more
semanticscholar +1 more source
RADIOACTIVE IRON RAIN: TRANSPORTING 60Fe IN SUPERNOVA DUST TO THE OCEAN FLOOR [PDF]
Several searches have found evidence of deposition, presumably from a near-Earth supernova (SN), with concentrations that vary in different locations on Earth.
Brian J. Fry, B. Fields, J. Ellis
semanticscholar +1 more source
Clustered supernovae as the sources of very-high-energy galactic cosmic rays
Although supernova remnants are believed to be the most plausible sources of galactic cosmic rays (CRs), it is yet unclear how they can accelerate particles beyond 1 PeV, especially when they evolve in the warm phase of the interstellar medium (ISM).
T. Vieu, B. Reville
semanticscholar +1 more source
The Cassiopeia A Supernova Was of Type IIb [PDF]
Cassiopeia A is the youngest supernova remnant known in the Milky Way and a unique laboratory for supernova physics. We present an optical spectrum of the Cassiopeia A supernova near maximum brightness, obtained from observations of a scattered light ...
O. Krause+6 more
semanticscholar +1 more source