dc.contributor.author | Thielemann, Friedrich-Karl | |
dc.contributor.author | Argast, D. | |
dc.contributor.author | Brachwitz, F. | |
dc.contributor.author | Martinez-Pinedo, Gabriel | |
dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Liebendoerfer, M. | |
dc.contributor.author | Mezzacappa, A. | |
dc.contributor.author | Hoflich, P. | |
dc.contributor.author | Iwamoto, K. | |
dc.contributor.author | Nomoto, K. | |
dc.contributor.editor | Fusco Femiano, R. | |
dc.contributor.editor | Matteucci, F. | |
dc.date.accessioned | 2014-11-27T09:14:31Z | |
dc.date.available | 2014-11-27T09:14:31Z | |
dc.date.issued | 2002 | |
dc.identifier.citation | Thielemann , F-K , Argast , D , Brachwitz , F , Martinez-Pinedo , G , Rauscher , T , Liebendoerfer , M , Mezzacappa , A , Hoflich , P , Iwamoto , K & Nomoto , K 2002 , Nucleosynthesis in supernovae . in R Fusco Femiano & F Matteucci (eds) , Chemical Enrichment of Intracluster and Intergalactic Medium . ASP Conf Series , vol. 253 , Astronomical Society of the Pacific , San Francisco , pp. 205-218 , Meeting on Chemical Enrichment of Intracluster and Intergalactic Medium , VULCANO , Italy , 14/05/01 . < http://www.aspbooks.org/publications/253/205.pdf > | |
dc.identifier.citation | conference | |
dc.identifier.isbn | 1-58381-093-5 | |
dc.identifier.isbn | 978-1-58381-589-2 | |
dc.identifier.uri | http://hdl.handle.net/2299/14824 | |
dc.description.abstract | The evolution of gas abundances in galaxies and the enrichment of heavy elements as a function of space and time reflects the history of star formation and the lifetimes of the diverse contributing stellar objects. Supernovae of type la and type II/Ib/Ic are the main contributors to nucleosynthesis in galaxies. Despite many efforts, a full and self-consistent understanding of supernova explosion mechanisms is not existing, yet. However, they leave fingerprints, seen either in spectra, lightcurves, radioactivities/decay gamma-rays or in galactic evolution. Here we want to address the relation of model uncertainties to the composition of ejecta and test them with constraints from abundance observations. | en |
dc.format.extent | 14 | |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | Chemical Enrichment of Intracluster and Intergalactic Medium | |
dc.relation.ispartofseries | ASP Conf Series | |
dc.subject | WEAK INTERACTION RATES | |
dc.subject | R-PROCESS NUCLEOSYNTHESIS | |
dc.subject | IA SUPERNOVAE | |
dc.subject | CARBON DEFLAGRATION SUPERNOVAE | |
dc.subject | II SUPERNOVAE | |
dc.subject | METAL-POOR STARS | |
dc.subject | ROTATING MASSIVE STARS | |
dc.subject | NEUTRINO-DRIVEN WINDS | |
dc.subject | CORE-COLLAPSE SUPERNOVAE | |
dc.subject | CIRCLE-DOT STAR | |
dc.title | Nucleosynthesis in supernovae | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.identifier.url | http://www.aspbooks.org/publications/253/205.pdf | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |