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The Supernova -- Supernova Remnant Connection [PDF]

open access: yes, 2017
Many aspects of the progenitor systems, environments, and explosion dynamics of the various subtypes of supernovae are difficult to investigate at extragalactic distances where they are observed as unresolved sources. Alternatively, young supernova remnants in our own galaxy and in the Large and Small Magellanic Clouds offer opportunities to resolve ...
Dan Milisavljevic, Robert A. Fesen
arxiv   +6 more sources

Supernovae and Supernova, Remnants

open access: bronzeThe Astronomical Journal, 1968
Supernovae remnants evolution, properties and galactic distribution, discussing criteria for catalog listing and remnants as X ray ...
Arcadio Poveda, L. Woltjer
openalex   +3 more sources

Supernova Remnants and their Supernovae [PDF]

open access: bronzeInternational Astronomical Union Colloquium, 1988
AbstractObserving supernova remnants provides important clues to the nature of supernova explosions. Conversely, the late stages of stellar evolution and the mechanism of supernova explosions affect supernova remnants through circumstellar matter, stellar remnants, and nucleosynthesis. The elements of supernova classification and the connection between
R. Kirshner
openalex   +3 more sources

Supernova 1987A: a Template to Link Supernovae to their Remnants [PDF]

open access: yesThe Astrophysical Journal, 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. Here we aim at identifying the imprint of SN 1987A on the X-ray emission of its remnant and at constraining the structure of ...
S. Orlando   +3 more
arxiv   +7 more sources

Supernova Remnants as Clues to Their Progenitors [PDF]

open access: yes, 2017
Supernovae shape the interstellar medium, chemically enrich their host galaxies, and generate powerful interstellar shocks that drive future generations of star formation. The shock produced by a supernova event acts as a type of time machine, probing the mass loss history of the progenitor system back to ages of $\sim$ 10 000 years before the ...
Carles Badenes, Daniel J. Patnaude
arxiv   +5 more sources

Multifrequency radio observations of a SNR in the LMC: The case of SNR J0527-6549 (DEM l204) [PDF]

open access: yesSerbian Astronomical Journal, 2010
We present a detailed study and results of new Australia Telescope Compact Array (ATCA) observations of supernova remnant SNR J0527-6549. This Large Magellanic Cloud (LMC) object follows a typical supernova remnant (SNR) horseshoe morphology ...
Bozzetto L.M.   +7 more
doaj   +3 more sources

Particle propagation in clumpy supernova remnants [PDF]

open access: yesEPJ Web of Conferences, 2019
The presence of dense clumps in the environment where a supernova remnant expands might have a strong impact in shaping the observed hadronic gamma-ray spectrum.
Celli Silvia
doaj   +1 more source

How Tycho Brahe’s recordings in 1572 support SN 1572 as a type I(a) supernova

open access: yesFrontiers in Astronomy and Space Sciences, 2023
The 450th anniversary of the discovery of the SN 1572 supernova event was celebrated in 2022. A closer look at the historical development of the field of supernova astronomy reveals the scientific importance of Tycho Brahe’s 1572 observations of this ...
Tobias C. Hinse   +5 more
doaj   +1 more source

A new numerical code for hydrodynamical 3D simulations of supernova remnants [PDF]

open access: yesSerbian Astronomical Journal, 2019
We develop a 3D hydrodynamical code written in C programming language to study the expansion of supernova remnants (SNRs) in the surrounding medium. It is based on the MUSCL-Hancock finite volume scheme with the HLLC Riemann solver.
Kostić P.
doaj   +1 more source

Electron–Ion Temperature Ratio in Astrophysical Shocks

open access: yesThe Astrophysical Journal, 2023
Collisionless shock waves in supernova remnants and the solar wind heat electrons less effectively than they heat ions, as is predicted by kinetic simulations.
John C. Raymond   +11 more
doaj   +1 more source

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