Results 201 to 210 of about 5,737 (225)
On the progenitors of core-collapse supernovae [PDF]
Astrophysics and Space Science, 2010 Theory holds that a star born with an initial mass between about 8 and 140 times the mass of the Sun will end its life through the catastrophic gravitational collapse of its iron core to a neutron star or black hole. This core collapse process is thought to usually be accompanied by the ejection of the star's envelope as a supernova.
exaly +3 more sources
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Anisotropies in Core Collapse Supernovae
Chinese Journal of Astronomy and Astrophysics, 2006Core-collapse supernovae are the final stage of the evolution of massive stars. When these have previously lost their hydrogen and helium envelopes, the supernova explosion is classified as Type Ic. This class of supernovae are particularly interesting because of the link with long-duration Gamma-Ray Bursts.
Pian, E., Mazzali, P.
openaire +2 more sources
AIP Conference Proceedings, 2007
In this contribution I highlight some of the new findings concerning core‐collapse, type II supernovae. In particular, after some comments on SN statistics, I review the case for a large spread in ejecta and Ni mass, the discovery of a population of faint, low energy events and the increasing evidences of the presence of dense circumstellar material ...
openaire +1 more source
In this contribution I highlight some of the new findings concerning core‐collapse, type II supernovae. In particular, after some comments on SN statistics, I review the case for a large spread in ejecta and Ni mass, the discovery of a population of faint, low energy events and the increasing evidences of the presence of dense circumstellar material ...
openaire +1 more source
Nucleosynthesis in core collapse supernovae
AIP Conference Proceedings, 1995Core-collapse supernovae (CCSNe) are one of the most important nucleosynthesis sites and they hold a key role in the evolution of galaxies. In the explosion, CCSNe eject freshly synthesized iron-group nuclei from explosive burning alongside of intermediate mass elements (from hydrostatic and explosive burning), and carbon and oxygen from the pre ...
F.-K. Thielemann +2 more
openaire +1 more source
Core-collapse supernovae and supernova neutrinos
23 pages, 8 figures. Preprint of a chapter for the Encyclopedia of Nuclear Physics, section Nuclear Astrophysics (ed. S.Mueller, B., Sykes, B.
openaire +1 more source
The Progenitors of Core-collapse Supernovae
AIP Conference Proceedings, 2009The first systematic searches for the progenitors of core‐collapse supernovae are now over a decade old. Exciting results from the detections, and even non‐detections, of the progenitors in archival pre‐explosion imaging have provided important clues to the role of processes in massive star evolution in the build up to SN explosion, as well as to the ...
Justyn R. Maund +7 more
openaire +1 more source
Hydrodynamics of core-collapse supernovae and their progenitors
Living Reviews in Solar Physics, 2020Bernhard Mueller, Müller Bernhard
exaly
The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae
Monthly Notices of the Royal Astronomical Society, 2020Alexander Heger +2 more
exaly
Long γ-ray bursts and core-collapse supernovae have different environments
Nature, 2006Andrew Levan +2 more
exaly