Results 21 to 30 of about 3,393,330 (216)
Detonation shock dynamics of Type Ia supernovae [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 The wavefront propagation of curved detonation waves in carbon–oxygen cores and helium shells of Type Ia supernova (SNIa) progenitors is determined via a detonation shock dynamics approach. A level set implementation is used to track the front, which is evolved according to intrinsic quasi-steady, quasi-one-dimensional detonation speed–curvature ...
Dunkley, SD, Sharpe, GJ, Falle, SAEG
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Topics in Core-Collapse Supernova Theory: The Formation of Black Holes and the Transport of Neutrinos [PDF]
, 2012 Core-Collapse Supernovae are one of the most complex astrophysical systems in the universe. They deeply entwine aspects of physics and astrophysics that are rarely side by side in nature.
O'Connor, Evan Patrick
core +1 more source
DYNAMICS OF AN ALFVÉN SURFACE IN CORE COLLAPSE SUPERNOVAE [PDF]
The Astrophysical Journal, 2011 18 pages, 14 figures, accepted for publication in ApJ.
Guilet, Jerome +2 more
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Arp 299-A: More than "just" a prolific supernova factory [PDF]
, 2010 We present partial results from our monitoring of the nuclear region of the starburst galaxy IC 694 (=Arp 299-A) at radio wavelengths, aimed at discovering recently exploded core-collapse supernovae, as well as to determine their rate of explosion, which
Marco Bondi +9 more
core +1 more source
Dirac-neutrino magnetic moment and the dynamics of a supernova explosion [PDF]
JETP Letters, 2009 10 pages, LaTeX, 4 EPS figures, accepted to JETP ...
Kuznetsov, A. V. +2 more
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Dynamics of radiative supernova remnants
The Astrophysical Journal, 1988 A high-resolution numerical simulation is used to study the evolution of a SNR evolving in a homogeneous uniform medium. Emphasis is placed on the transition from the adiabatic stage to the radiative pressure-driven snowplow stage, along with the possible further establishment of a momentum-conserving snowplow state.
Denis F. Cioffi +2 more
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Core-collapse Supernova Explosions in Active Galactic Nucleus Accretion Disks
The Astrophysical Journal, 2023 Astrophysical events that occur in active galactic nucleus (AGN) disks are believed to differ significantly from the ordinary in the interstellar medium.
Fu-Lin Li +6 more
doaj +1 more source
Dynamics of Fe Bubbles in Young Supernova Remnants [PDF]
The Astrophysical Journal, 2001 Observations of core-collapse supernovae (SNe) have revealed the presence of extensive mixing of radioactive material in SN ejecta. The mixing of radioactive material, mostly freshly synthesized Ni, is not complete, which leads to a two-phase SN ejecta structure. The low-density phase consists of Fe bubbles, created by the energy input from radioactive
Blondin, J. M. +2 more
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Neutrino-nucleus reactions in supernovae
EPJ Web of Conferences, 2016 We study thermal effects on neutrino-nucleus reactions occurring under supernova conditions. The approach we use is based on the QRPA extended to finite temperature by the thermofield dynamics formalism. For the relevant supernova conditions we calculate
Dzhioev Alan A., Vdovin A.I.
doaj +1 more source