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X-Ray Measured Dynamics of Tycho's Supernova Remnant [PDF]
Astrophysical Journal, 2010 We present X-ray proper-motion measurements of the forward shock and reverse-shocked ejecta in Tycho's supernova remnant, based on three sets of archival Chandra data taken in 2000, 2003, and 2007. We find that the proper motion of the edge of the remnant (i.e., the forward shock and protruding ejecta knots) varies from 0".20 yr^{-1} (expansion index m=
Satoru Katsuda +2 more
exaly +3 more sources
Neutrino–Nucleus Reactions and Their Role for Supernova Dynamics and Nucleosynthesis [PDF]
Progress in Particle and Nuclear Physics, 2015 77 pages, 29 figures, 4 tables, submitted to Progress in Particle and Nuclear ...
Gabriel Martínez-Pinedo, K Langanke
exaly +3 more sources
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Non-Linear Dynamics of the Richtmyer–Meshkov Instability in Supernovae
Astrophysics and Space Science, 2005zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Abarzhi, Snezhana I., Herrmann, Marcus
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Dynamics of bubbles in supernovae and turbulent vortices
Astronomy Reports, 2006We consider the motion of a bubble in a central acceleration field created by gravity or a centrifugal force. In the former case, the bubble moves outwards from and, in the latter, towards the center. We have calculated the characteristic time needed for a bubble to leave or reach the center. The solution obtained provides insight into the processes of
V. Bychkov +4 more
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The Dynamics of Supernova Envelopes
1987The dynamics and radiative emission of supernovae are reviewed from the supernova explosion up to the early remnant stage.
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The dynamical effects of supernovae on the interstellar medium
Astrophysics and Space Science, 1975An interstellar cloud suddenly overrun by a supernova blast wave experiences a very rapid increase in boundary pressure. A shock wave propagates into the cloud. As a preliminary investigation, the propagation of spherical shock waves in an adiabatic medium is studied numerically.
J. E. Dyson, P. Gulliford
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Classical and Quantum Gravity, 2010
Summary: In contrast to heavy ion collisions, matter in astrophysical systems such as neutron stars, compact star mergers and supernova environments can be highly isospin asymmetric. We focus on core collapse supernova matter where temperatures reach tens of MeV.
T. Fischer +5 more
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Summary: In contrast to heavy ion collisions, matter in astrophysical systems such as neutron stars, compact star mergers and supernova environments can be highly isospin asymmetric. We focus on core collapse supernova matter where temperatures reach tens of MeV.
T. Fischer +5 more
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The dynamic evolution of the Kepler supernova remnant
Astrophysics and Space Science, 1986Two supernovae exploding events were observed visually from the same position, the north of Tian-Jiang in Wei-Suei (the north of 42 θ Ophiuchi), in 1604 and 1664, respectively, and were recorded in the ancient astronomical literatures of China and Korea.
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Dynamics of Supernova Explosion
AIP Conference Proceedings, 2008V. M. Chechetkin +6 more
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