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Supernova Remnants: Types and Evolution
Although only a small fraction of stars end their lives as supernovae, all supernovae leave behind a supernova remnant (SNR), an expanding shock wave...
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Thermal Processes in Supernova Remnants
This chapter provides a theoretical overview of thermal processes in supernova remnants (SNRs), which can be understood as a series of energy...
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Thermal Processes in Supernova Remnants
This chapter provides a theoretical overview of thermal processes in supernova remnants (SNRs), which can be understood as a series of energy...
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Nonthermal Processes and Particle Acceleration in Supernova Remnants
Shocks of supernova remnants (SNRs) accelerate charged particles up to ∼100 TeV range via diffusive shock acceleration (DSA) mechanism. It is...
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Supernova Remnants: Types and Evolution
Although only a small fraction of stars end their lives as supernovae, all supernovae leave behind a supernova remnant (SNR), an expanding shock wave...
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Detection possibilities of hostless intergalactic supernova remnants with Square Kilometre Array
Possibilities to detect hostless supernova remnants (hl-SNR) in intergalactic medium using the 1 GHz band of the Square Kilometre Array (SKA) are...
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Nonthermal Processes and Particle Acceleration in Supernova Remnants
Shocks of supernova remnants (SNRs) accelerate charged particles up to ∼100 TeV range via diffusive shock acceleration (DSA) mechanism. It is...
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Radio Emission Variability of Supernova Remnants and a Possible Explanation of the Phenomenon
AbstractThe flux densities and current spectra of plerions and combined supernova remnants (SNRs): 3C58, 3C144, G11.2–0.3, G21.5–0.9, and 3C396 are...
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Peering into the Milky Way by FAST: IV. Identification of two new Galactic supernova remnants G203.1+6.6 and G206.7+5.9
A5° × 7° sky area containing two large radio structures of G203.1+6.6 and G206.7+5.9 with a size of about 2°.5 and 3°.5 respectively is scanned by...
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The Relationship Between Supernova Remnants and Neutron Stars
We comment briefly on facts and ideas concerning the relationship between neutron stars and supernova remnants and the role of the stellar magnetic...
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Patterns in the Chaos: An Unsupervised View of Galactic Supernova Remnants
Supernova Remnants (SNRs) constitute a remarkably heterogeneous population that exhibits a wide variety of observational properties. These...
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Cosmic Ray Acceleration in Supernova Remnants with Nonuniform Density Distribution
AbstractA study is performed of the acceleration of cosmic rays by shock waves propagating in bubbles of hot rarefied gas created by the stellar wind...
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High-Resolution X-Ray Spectroscopy of Supernova Remnants
Thermal X-ray spectra from supernova remnants (SNRs) are dominated by a number of line emission from various elements. Resolving the individual lines...
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Study of the Influence of the Background Neutral Component on the Dynamics of the Envelope in Supernova Remnants
AbstractThe influence of neutrals on the development of multidimensional dense-shell instabilities in supernova remnants is investigated. We present...
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Magnetorotational Supernova Neutrino Emission Spectra and Prospects for Observations by Large-Size Underwater Telescopes
AbstractWe analyze neutrino fluxes near the surface of a protoneutron star in type II supernova explosions. For magnetorotational explosion mechanism...
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Optical Emission from Supernova Remnants
Several Galactic supernova remnants were known to astronomers as optical nebulae, long before the concept of supernovae and supernova remnants were...
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Physics and Evolution of Supernova Remnants
Written by a leading expert, this monograph presents recent developments on supernova remnants, with the inclusion of results from various satellites...
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Collisional Pum** of OH Masers near Supernova Remnants
AbstractThe collisional pum** of OH masers in non-dissociative C-type shocks near supernova remnants is considered. The emergence of maser emission...
