Results 21 to 30 of about 101,525 (149)

The Thousand-Pulsar-Array programme on MeerKAT - X. Scintillation arcs of 107 pulsars [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2022
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

The nearest neutron star candidate in a binary revealed by optical time-domain surveys [PDF]

open access: yesScience China Physics Mechanics and Astronomy, 2022
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]

open access: yesAstrophysical Journal, 2018
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]

open access: yesJournal of Physics: Conference Series, 2019
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

Phosphorus in the Young Supernova Remnant Cassiopeia A [PDF]

open access: yesScience, 2013
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]

open access: yes, 2016
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

Recent near-Earth supernovae probed by global deposition of interstellar radioactive 60Fe

open access: yesNature, 2016
The rate of supernovae in our local Galactic neighbourhood within a distance of about 100 parsecs from Earth is estimated to be one every 2–4 million years, based on the total rate in the Milky Way (2.0 ± 0.7 per century).
A. Wallner   +14 more
semanticscholar   +1 more source

Flavor composition of supernova neutrinos [PDF]

open access: yesPhysical Review D
Predicting the flavor composition of neutrinos from supernovae is a challenging task, primarily due to the high neutrino densities at their core. In such an environment, neutrino self-interactions give rise to collective effects that have dramatic yet ...
Antonio Capanema   +2 more
semanticscholar   +1 more source

The Cassiopeia A Supernova Was of Type IIb [PDF]

open access: yesScience, 2008
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

Clustered supernovae as the sources of very-high-energy galactic cosmic rays

open access: yesInternational Conference on Rebooting Computing, 2023
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

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