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By Wolfgang Hillebrandt, Rudolf Kuhfuß, Ewald Müller, JamesW. Truran

The new discovery of a sort II supernova within the huge Magellanic Cloud offers a unprecedented probability to match types of stellar evolution and nucleosynthesis at once with observations. This workshop covers thermonuclear response premiums in chaos (experimental and theoretical), stellar evolution, nucleosynthesis and isotopic anomalies in meteorites and, in a last part, the supernovae, particularly SN 1987A. It brings the main fascinating information within the swiftly constructing box of nuclear astrophysics to researchers and likewise to graduate scholars. fresh and destiny advancements are mentioned. detailed emphasis is put on experimental and theoretical methods to acquiring nuclear response premiums, types of stellar evolution and explosions, and theories of nucleosynthesis. quite a few features of stellar evolution, nucleosynthesis, and thermonuclear reactions of astrophysical curiosity are reviewed. numerous contributions take care of supernova explosions of big stars, and specifically with Supernova 1987A and its effect on present types of the evolution of huge stars, the gravitational cave in of stellar cores, and neutrino physics and astronomy.

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E. Pollock: Annu. Rev. Nucl. Part. Sci. 41, 357 (1991) 28. D. Habs, W. Baumann, J. Berger, P. Blatt, A. Faulstich, P. Krause, G. Kilgus, R. Neumann, W. Petrich, R. Stockstad, D. Schwalm, E. Szmola, K. Welti, A. Wolf, S. Zwickler, E. Jaeschke, D. Kramer, G. Bisoffi, M. Blum, A. Friedrich, C. Geyer, M. -W. Heyng, B. Holzer, R. Ihde, M. Jung, K Matl, W. Ott, B. Povh, R. Repnow, M. Steck, E. Steffens, D. Dutta, T. Kuhl, D. Marx, S. Schroder, M. Gerhard, R. Grieser, G. Huber, R. Klein, M. Krieg, N. Schmidt, R.

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Wolf: Phys. Rev. Lett. 75, 802 (1995) 75. S. Borneis, F. Bosch, T. Engel, M. Jung, I. Klaft, T. Kuhl, D. Marx R. Moshammer, R. Neumann, S. Schroder, P. Seelig, L. VOlker: Phys. Rev. Lett. G. Schneider, J. Steiger, T. R. Crespo Lopez-Urrutia Summary. Two Electron Beam Ion Traps (EBIT) , the low energy EBIT II (40 keY electron beam energy) and the high-energy Super EBIT (200 keY electron beam energy) at Lawrence Livermore National Laboratory produce the highest charge state ions of any element (up to U92 +).

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