Results 201 to 210 of about 5,709 (225)

Extreme energy in a relaxed galaxy group indicates the bursty nature of AGN feedback

Eckert D, Gastaldello F, Lovisari L, McGee S, Pasini T, Brienza M, Kolokythas K, O'Sullivan E, Simionescu A, Sun M, Bourne M, Chen Y, Cui W, Ettori S, Finoguenov A, Gozaliasl G, Kale R, Mernier F, Oppenheimer B, Schellenberger G, Seppi R, Tempel E.   +21 more
europepmc   +1 more source

Core-Collapse Supernovae, Neutrinos, and Gravitational Waves [PDF]

Nuclear Physics, Section B, Proceedings Supplements, 2013
Core-collapse supernovae are among the most energetic cosmic cataclysms. They are prodigious emitters of neutrinos and quite likely strong galactic sources of gravitational waves.
S Gossan, Ernazar Abdikamalov
exaly   +1 more source

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Anisotropies in Core Collapse Supernovae

Chinese Journal of Astronomy and Astrophysics, 2006
Core-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

Core collapse supernovae

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 ...
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Nucleosynthesis in core collapse supernovae

AIP Conference Proceedings, 1995
Core-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, Ken’ichi Nomoto, Masaaki Hashimoto   +2 more
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The Progenitors of Core-collapse Supernovae

AIP Conference Proceedings, 2009
The 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, Giuliana Giobbi, Amedeo Tornambe, Gabriella Raimondo, Marco Limongi, L. A. Antonelli, Nicola Menci, Enzo Brocato   +7 more
openaire   +1 more source

Hydrodynamics of core-collapse supernovae and their progenitors

Living Reviews in Solar Physics, 2020
Bernhard Müller, Müller Bernhard
exaly  

Gravitational Waves from Core-Collapse Supernovae

2022
Ernazar Abdikamalov, David Radice, Radice David   +2 more
exaly  

The impact of fallback on the compact remnants and chemical yields of core-collapse supernovae

Monthly Notices of the Royal Astronomical Society, 2020
Conrad Chan, Bernhard Müller, Alexander Heger   +2 more
exaly  

Long γ-ray bursts and core-collapse supernovae have different environments

Nature, 2006
P M Vreeswijk, S E Thorsett, J M Castro Ceron   +2 more
exaly