How high energy fluxes may affect Rayleigh–Taylor instability growth in young supernova remnants [PDF]
Nature Communications, 2018 Radiation and conduction are generally considered as the main energy transport mechanisms for the evolution of early supernova remnants. Here the authors experimentally show the role of electron heat transfer on the growth of Rayleigh–Taylor instability ...
C. C. Kuranz +27 more
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Asymmetric supernova remnants generated by Galactic, massive runaway stars [PDF]
, 2015 After the death of a runaway massive star, its supernova shock wave interacts with the bow shocks produced by its defunct progenitor, and may lose energy, momentum, and its spherical symmetry before expanding into the local interstellar medium (ISM).
Gusdorf, A. +4 more
core +3 more sources
The supernova remnant SN 1006 as a Galactic particle accelerator [PDF]
Nature Communications, 2022 It is known that cosmic rays could be accelerated by shock waves in supernova (SN) remnants. Here, the authors show that SN 1006 remnant is an efficient source of cosmic rays, providing observational support for the quasi-parallel acceleration mechanism.
Roberta Giuffrida +8 more
doaj +2 more sources
Progenitors of Recombining Supernova Remnants [PDF]
, 2012 Usual supernova remnants have either ionizing plasma or plasma in collisional ionization equilibrium, i.e., the ionization temperature is lower than or equal to the electron temperature.
Blinnikov +22 more
core +2 more sources
Supernova 1987A: a Template to Link Supernovae to their Remnants [PDF]
, 2015 The emission of supernova remnants reflects the properties of both the progenitor supernovae and the surrounding environment. The complex morphology of the remnants, however, hampers the disentanglement of the two contributions.
Bocchino, F. +3 more
core +4 more sources
Revised Distances to 21 Supernova Remnants [PDF]
, 2018 We carry out a comprehensive study of H i 21 cm line observations and 13CO line observations of 21 supernova remnants (SNRs). The aim of the study is to search for H i absorption features to obtain kinematic distances in a consistent manner.
S. Ranasinghe, D. A. Leahy
openalex +3 more sources
Acceleration of cosmic rays and gamma-ray emission from supernova remnants in the Galaxy [PDF]
, 2013 Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Though very popular and robust, this conjecture still needs a conclusive proof.
Casanova, S. +4 more
core +4 more sources
The Hunt for Pevatrons: The Case of Supernova Remnants [PDF]
Universe, 2021 The search for Galactic pevatrons is now a well-identified key science project of all instruments operating in the very-high-energy domain. Indeed, in this energy range, the detection of gamma rays clearly indicates that efficient particle acceleration ...
P. Cristofari
semanticscholar +1 more source
Searches for Continuous Gravitational Waves from Young Supernova Remnants in the Early Third Observing Run of Advanced LIGO and Virgo [PDF]
, 2021 We present results of three wide-band directed searches for continuous gravitational waves from 15 young supernova remnants in the first half of the third Advanced LIGO and Virgo observing run.
semanticscholar +1 more source
Dynamics of millicharged dark matter in supernova remnants [PDF]
Physical Review D, 2020 Dark matter could have a small electromagnetic charge, provided the charge-to-mass ratio is much less than that of electrons or protons. This candidate, commonly known as millicharged dark matter (mDM), would form a plasma and interact with the ...
Jung-Tsung Li, Tongyan Lin
semanticscholar +1 more source