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Titlebook: Mathematik für Wirtschaftswissenschaftler; Intuitiv und praxisn Bertil Haack,Ulrike Tippe,Tilo Wendler Textbook 2017 Springer-Verlag GmbH D

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41#
發(fā)表于 2025-3-28 16:32:20 | 只看該作者
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendlerd, e.g., neutron star mergers and (sub-classes) of supernovae (e.g., [.,.,.,.]). .-process elements have been measured in a large fraction of metal-poor stars [.]. Galactic archeology studies show that the r-process abundances among these stars vary by over two orders of magnitude. On the other hand
42#
發(fā)表于 2025-3-28 20:53:19 | 只看該作者
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendlerd, e.g., neutron star mergers and (sub-classes) of supernovae (e.g., [.,.,.,.]). .-process elements have been measured in a large fraction of metal-poor stars [.]. Galactic archeology studies show that the r-process abundances among these stars vary by over two orders of magnitude. On the other hand
43#
發(fā)表于 2025-3-29 02:14:52 | 只看該作者
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendlerd, e.g., neutron star mergers and (sub-classes) of supernovae (e.g., [.,.,.,.]). .-process elements have been measured in a large fraction of metal-poor stars [.]. Galactic archeology studies show that the r-process abundances among these stars vary by over two orders of magnitude. On the other hand
44#
發(fā)表于 2025-3-29 05:33:48 | 只看該作者
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendlerd, e.g., neutron star mergers and (sub-classes) of supernovae (e.g., [.,.,.,.]). .-process elements have been measured in a large fraction of metal-poor stars [.]. Galactic archeology studies show that the r-process abundances among these stars vary by over two orders of magnitude. On the other hand
45#
發(fā)表于 2025-3-29 08:17:59 | 只看該作者
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendlerd, e.g., neutron star mergers and (sub-classes) of supernovae (e.g., [.,.,.,.]). .-process elements have been measured in a large fraction of metal-poor stars [.]. Galactic archeology studies show that the r-process abundances among these stars vary by over two orders of magnitude. On the other hand
46#
發(fā)表于 2025-3-29 12:18:12 | 只看該作者
47#
發(fā)表于 2025-3-29 17:27:02 | 只看該作者
Bertil Haack,Ulrike Tippe,Michael Stobernack,Tilo Wendlerd from all kinds of nuclear reactions, including measurements of reactions with neutrons and γ-rays not yet fully considered in previous compilations. The nuclei considered also comprise nuclei far from the stability line..?.The properties of excited nuclear states are of importance for scientific a
48#
發(fā)表于 2025-3-29 20:37:35 | 只看該作者
d from all kinds of nuclear reactions, including measurements of reactions with neutrons and γ-rays not yet fully considered in previous compilations. The nuclei considered also comprise nuclei far from the stability line..?.The properties of excited nuclear states are of importance for scientific a
49#
發(fā)表于 2025-3-30 03:35:56 | 只看該作者
Modellieren und Argumentieren,iengang studieren und in diesem Zusammenhang mit wirtschaftswissenschaftlichen Fragestellungen konfrontiert werden, die Sie l?sen sollen und im besten Fall auch l?sen wollen. Es kann auch sein, dass Sie bereits berufst?tig sind und wirtschaftswissenschaftliche Aufgaben aus der Praxis auf Sie warten.
50#
發(fā)表于 2025-3-30 07:44:17 | 只看該作者
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