Results 31 to 40 of about 31,180 (215)

Nucleosynthesis in Core Collapse Supernovae

AIP Conference Proceedings, 2006
PDF Document, 6 pages, 2 figures. . Proceedings of "Origin of Matter and Evolution of Galaxies (OMEG05): New Horizon of Nuclear Astrophysics and Cosmology".
Limongi, M., Chieffi, A.
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Multimessenger asteroseismology of core-collapse supernovae [PDF]

Physical Review D, 2019
25 pages, 16 figures. Version accepted to PRD.
John Ryan Westernacher-Schneider, Evan O’Connor, Erin O’Sullivan, Irene Tamborra, Meng-Ru Wu, Sean M. Couch, Felix Malmenbeck   +6 more
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The physics of core-collapse supernovae [PDF]

Nature Physics, 2005
Review article; 17 pages, 5 ...
Woosley, S., Janka, T.
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Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf

The Astrophysical Journal Letters, 2023
Stellar evolution theory predicts multiple pathways to the explosive deaths of stars as supernovae. Locating and characterizing the progenitors of well-studied supernovae is important to constrain the theory and to justify and design future surveys to ...
Joanne L Pledger, Michael M Shara
doaj   +1 more source

Nuclei in core-collapse supernovae engine

Progress in Particle and Nuclear Physics, 2023
Herein, we review the nuclear equations of state (EOSs) %for core-collapse supernova simulations and the constituent nuclei of core-collapse supernovae (CCSNe) and their roles in CCSN simulations. Various nuclei such as deuterons, iron, and extremely neutron-rich nuclei compose in the central engines of CCSNe.
S. Furusawa, H. Nagakura
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The Iron Yield of Core-collapse Supernovae

The Astrophysical Journal, 2023
We present a systematic analysis of 191 stripped-envelope supernovae (SE SNe), aimed at computing their ^56 Ni masses from the luminosity in their radioactive tails ( ${M}_{\mathrm{Ni}}^{\mathrm{tail}}$ ) and/or in their maximum light, and the mean ^56 ...
Ósmar Rodríguez, Dan Maoz, Ehud Nakar
doaj   +1 more source

Strange matter in core-collapse supernovae

ACTA PHYSICA POLONICA B, 2011
8 pages, 3 figures, Invited talk at the "Strangeness in Quark Matter" conference, 18-24 September 2011, Polish Academy of Arts and Sciences, Cracow ...
I. Sagert, T. Fischer, M. Hempel, PAGLIARA, Giuseppe, J. Schaffner Bielich, F. K. Thielemann, M. Liebendörfer   +6 more
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The demographics of core-collapse supernovae

Astronomy & Astrophysics
Context. The observational properties of core-collapse supernovae are shaped by the envelopes of their progenitors. In massive binary systems, mass-transfer drastically alters the pre-supernova structures compared to single stars, which leads to a ...
Ercolino Andrea, Jin Harim, Langer Norbert, Gal-Yam Avishay, Schootemeijer Abel, Mannes Caroline   +5 more
doaj   +1 more source

A low energy core-collapse supernova without a hydrogen envelope [PDF]

, 2009
The final fate of massive stars depends on many factors, including mass, rotation rate, magnetic fields and metallicity. Theory suggests that some massive stars (initially greater than 25-30 solar masses) end up as Wolf-Rayet stars which are deficient in
A Filippenko, A Gal-Yam, A Heger, A Pastorello, A Pastorello, A. Harutyunyan, A. Pastorello, AI MacFadyen, AV Filippenko, AV Filippenko, CL Fryer, D Branch, DK Sahu, E. Cappellaro, E. Pian, F Patat, FS Kitaura, J. Manteca, JPU Fynbo, K Nomoto, K Nomoto, L. Zampieri, M Della Valle, M. Nissinen, M. Turatto, MM Phillips, MM Phillips, N. Elias-Rosa, P. A. Mazzali, PA Mazzali, PA Mazzali, R. Ferrando, S Benetti, S Jha, S Valenti, S. Benetti, S. J. Smartt, S. Taubenberger, S. Valenti, T Matheson, V. P. Hentunen, VN Gamezo, W Li, WD Arnett   +43 more
core   +2 more sources

Young Core‐Collapse Supernova Remnants and Their Supernovae [PDF]

The Astrophysical Journal, 2005
43 pages, ApJ, revised, discussion of 3C58 changed, in press for Feb.
openaire   +2 more sources