Nucleosynthesis modes in the high-entropy-wind of type II supernovae
Authors:
- K.-L. KratzKKK.-L. Kratz
- K. FarouqiKFK. Farouqi
- L.I. MashonkinaLML.I. Mashonkina
- B. PfeifferBPB. Pfeiffer
- 1 October 2008
- journal article
- review article
- Published by Elsevier in New Astronomy Reviews
- Vol. 52 (7-10) , 390-395
Abstract
No abstract availableKeywords
This publication has 48 references indexed in Scilit:
- Features of the Acoustic Mechanism of Core‐Collapse Supernova ExplosionsThe Astrophysical Journal, 2007
- Neutrino opacities in nuclear matterNuclear Physics A, 2006
- Heavy element synthesis in the oldest stars and the early UniverseNature, 2006
- The Hamburg/ESO R-process enhanced star survey (HERES)Astronomy & Astrophysics, 2005
- Hubble Space TelescopeObservations of Heavy Elements in Metal‐Poor Galactic Halo StarsThe Astrophysical Journal, 2005
- Neutron star mergers versus core-collapse supernovae as dominant r-process sites in the early GalaxyAstronomy & Astrophysics, 2004
- First stars V - Abundance patterns from C to Zn and supernova yields in the early GalaxyAstronomy & Astrophysics, 2004
- Neutron Capture in Low‐Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance SignaturesThe Astrophysical Journal, 1999
- The R-process and nucleochronologyPhysics Reports, 1991
- Synthesis of the Elements in StarsReviews of Modern Physics, 1957