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Titlebook: Astronomy with Radioactivities; Roland Diehl,Dieter H. Hartmann,Nikos Prantzos Book 20111st edition Springer-Verlag Berlin Heidelberg 2011

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31#
發(fā)表于 2025-3-26 22:41:52 | 只看該作者
32#
發(fā)表于 2025-3-27 04:59:47 | 只看該作者
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發(fā)表于 2025-3-27 06:00:22 | 只看該作者
Burkhard Kommerell,Peter Hahn,Ellen Webern of (a)?(magneto-)hydrodynamics, (b)?energy generation due to nuclear reactions accomanying composition changes, (c)?radiation transport, (d)?thermodynamic properties (such as the equation of state of stellar matter).
34#
發(fā)表于 2025-3-27 12:37:16 | 只看該作者
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M. Kaltenbach,B. Kunkel,M. Schneider could only be responsible for mild explosions, like novae, as a consequence of the necessity to convert two protons into two neutrons, and that only the thermonuclear fusion of carbon could be energetic enough to feed a strong explosion. They did not consider helium because by this epoch the He-bur
37#
發(fā)表于 2025-3-27 23:06:06 | 只看該作者
H. P. Krayeilbühl,P. Eichhorn,F. Horns of galactic nucleosynthesis, and/or of local processes (either exotic or in-situ) preceding and accompanying the formation of the Sun. This will also need some reference to the present scenarios for star formation, as applied to the ESS.
38#
發(fā)表于 2025-3-28 03:51:16 | 只看該作者
Technik moderner Schrittmacher-Systeme detectable. The large number of degrees of freedom that may be present in the microscopic physics must be explored by clever variations of the experimental setup. Most astronomical observations are obviously also taken from the far field, because the distance to the observed source is so much large
39#
發(fā)表于 2025-3-28 08:53:16 | 只看該作者
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