scholarly journals The bubble-like interior of the core-collapse supernova remnant Cassiopeia A

Science ◽  
2015 ◽  
Vol 347 (6221) ◽  
pp. 526-530 ◽  
Author(s):  
D. Milisavljevic ◽  
R. A. Fesen
Keyword(s):  
Supernova Remnant ◽  
Core Collapse ◽  
Cassiopeia A ◽  
Core Collapse Supernova ◽  
The Core

THE PUZZLING JET AND PULSAR WIND NEBULA OF IGR J11014-6103

2014 ◽  
Vol 28 ◽  
pp. 1460172 ◽  
Author(s):  
LUCIA PAVAN ◽  
POL BORDAS ◽  
GERD PÜHLHOFER ◽  
MIROSLAV D. FILIPOVIC ◽  
AIN DE HORTA ◽  
...  
Keyword(s):  
Neutron Star ◽  
Supernova Remnant ◽  
Helical Structure ◽  
Core Collapse ◽  
Radio Observations ◽  
X Ray ◽  
Core Collapse Supernova ◽  
The Core ◽  
Pulsar Wind

IGR J11014-6103 is a hard X-ray source discovered by INTEGRAL. Follow-up X-ray and radio observations revealed an elongated pulsar wind nebula formed by a neutron star escaping supersonically its parent supernova remnant SNR MSH 11-61A. The pulsar also emits highly collimated jets extending perpendicularly to the direction of motion. The jet has a continuous helical structure extending up to more than 10 parsecs. IGR J11014-6103 is a laboratory to study jet ejection in the wind of a pulsar and to constrain the core collapse supernova mechanism responsible for the observed pulsar kick velocity in excess of 1000 km/s.

scholarly journals DENSE IRON EJECTA AND CORE-COLLAPSE SUPERNOVA EXPLOSION IN THE YOUNG SUPERNOVA REMNANT G11.2-0.3

2009 ◽  
Vol 703 (1) ◽  
pp. L81-L85 ◽  
Author(s):  
Dae-Sik Moon ◽  
Bon-Chul Koo ◽  
Ho-Gyu Lee ◽  
Keith Matthews ◽  
Jae-Joon Lee ◽  
...  
Keyword(s):  
Supernova Remnant ◽  
Supernova Explosion ◽  
Core Collapse ◽  
Core Collapse Supernova ◽  
Young Supernova Remnant

scholarly journals The core collapse supernova rate from 24 years of data of the Large Volume Detector

2017 ◽  
Vol 888 ◽  
pp. 012256 ◽  
Author(s):  
G. Bruno ◽  
W. Fulgione ◽  
A. Molinario ◽  
C. Vigorito ◽  
Keyword(s):  
Large Volume ◽  
Core Collapse ◽  
Core Collapse Supernova ◽  
The Core ◽  
Large Volume Detector

scholarly journals THE CORE COLLAPSE SUPERNOVA RATE FROM THE SDSS-II SUPERNOVA SURVEY

2014 ◽  
Vol 792 (2) ◽  
pp. 135 ◽  
Author(s):  
Matt Taylor ◽  
David Cinabro ◽  
Ben Dilday ◽  
Lluis Galbany ◽  
Ravi R. Gupta ◽  
...  
Keyword(s):  
Core Collapse ◽  
Core Collapse Supernova ◽  
The Core

scholarly journals X-RAY EJECTA KINEMATICS OF THE GALACTIC CORE-COLLAPSE SUPERNOVA REMNANT G292.0+1.8

2015 ◽  
Vol 800 (1) ◽  
pp. 65 ◽  
Author(s):  
Jayant Bhalerao ◽  
Sangwook Park ◽  
Daniel Dewey ◽  
John P. Hughes ◽  
Koji Mori ◽  
...  
Keyword(s):  
Supernova Remnant ◽  
Core Collapse ◽  
X Ray ◽  
Core Collapse Supernova

scholarly journals Thoughts on Core-Collapse Supernova Theory

2007 ◽  
Vol 3 (S250) ◽  
pp. 185-192 ◽  
Author(s):  
Adam Burrows ◽  
Luc Dessart ◽  
Christian D. Ott ◽  
Eli Livne ◽  
Jeremiah Murphy
Keyword(s):  
Spherical Symmetry ◽  
State Of The Art ◽  
Core Collapse ◽  
Core Collapse Supernova ◽  
The Core ◽  
Heating Mechanism ◽  
Numerical Tools ◽  
Computational Resources ◽  
Do So

AbstractAn emerging conclusion of theoretical supernova research is that the breaking of spherical symmetry may be the key to the elusive mechanism of explosion. Such explorations require state-of-the-art multi-dimensional numerical tools and significant computational resources. Despite the thousands of man-years and thousands of CPU-years devoted to date to studying the supernova mystery, both require further evolution. There are many computationally-challenging instabilities in the core, before, during, and after the launch of the shock, and a variety of multi-dimensional mechanisms are now being actively explored. These include the neutrino heating mechanism, the MHD jet mechanism, and an acoustic mechanism. The latter is the most controversial, and, as with all the contenders, requires detailed testing and scrutiny. In this paper, we analyze recent attempts to do so, and suggests methods to improve them.

scholarly journals Three-dimensional models of core-collapse supernovae from low-mass progenitors with implications for Crab

2020 ◽  
Vol 496 (2) ◽  
pp. 2039-2084 ◽  
Author(s):  
G Stockinger ◽  
H-T Janka ◽  
D Kresse ◽  
T Melson ◽  
T Ertl ◽  
...  
Keyword(s):  
Three Dimensional ◽  
Iron Core ◽  
Core Collapse ◽  
Crab Pulsar ◽  
Core Collapse Supernova ◽  
Spin Period ◽  
The Core ◽  
Low Mass ◽  
Catch Up ◽  
Three Dimensional Models

ABSTRACT We present 3D full-sphere supernova simulations of non-rotating low-mass (∼9 M⊙) progenitors, covering the entire evolution from core collapse through bounce and shock revival, through shock breakout from the stellar surface, until fallback is completed several days later. We obtain low-energy explosions (∼0.5–1.0 × 1050 erg) of iron-core progenitors at the low-mass end of the core-collapse supernova (LMCCSN) domain and compare to a super-AGB (sAGB) progenitor with an oxygen–neon–magnesium core that collapses and explodes as electron-capture supernova (ECSN). The onset of the explosion in the LMCCSN models is modelled self-consistently using the vertex-prometheus code, whereas the ECSN explosion is modelled using parametric neutrino transport in the prometheus-HOTB code, choosing different explosion energies in the range of previous self-consistent models. The sAGB and LMCCSN progenitors that share structural similarities have almost spherical explosions with little metal mixing into the hydrogen envelope. A LMCCSN with less second dredge-up results in a highly asymmetric explosion. It shows efficient mixing and dramatic shock deceleration in the extended hydrogen envelope. Both properties allow fast nickel plumes to catch up with the shock, leading to extreme shock deformation and aspherical shock breakout. Fallback masses of $\mathord {\lesssim }\, 5\, \mathord {\times }\, 10^{-3}$ M⊙ have no significant effects on the neutron star (NS) masses and kicks. The anisotropic fallback carries considerable angular momentum, however, and determines the spin of the newly born NS. The LMCCSN model with less second dredge-up results in a hydrodynamic and neutrino-induced NS kick of >40 km s−1 and a NS spin period of ∼30 ms, both not largely different from those of the Crab pulsar at birth.

scholarly journals Detailed X-Ray Mapping of the Shocked Ejecta and Circumstellar Medium in the Galactic Core-collapse Supernova Remnant G292.0+1.8

2019 ◽  
Vol 872 (1) ◽  
pp. 31 ◽  
Author(s):  
Jayant Bhalerao ◽  
Sangwook Park ◽  
Andrew Schenck ◽  
Seth Post ◽  
John P. Hughes
Keyword(s):  
Supernova Remnant ◽  
Core Collapse ◽  
X Ray ◽  
Core Collapse Supernova ◽  
Circumstellar Medium
Sign in / Sign up

Export Citation Format

Share Document