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2 Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth What is the bulk composition of the solar system? Where/when/how did the atoms
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ABSTRACT INTRODUCTION METHODS DISCUSSION AND CONCLUSIONS Sediment cores were taken from Decodon Pond wetland using a Livingston corer, and from Jamaica
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The s-process Fe Co Ni Rb Ga Ge Zn Cu Se Br As Zr Y Sr Kr (n, ) ()() ()() r-process p-process 63 Ni, t 1/2 =100 a 64 Cu, t 1/2 =12 h, 40 % (
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Lecture 15 Explosive Nucleosynthesis and the r-Process
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Danica Kačíková Katedra protipožiarnej ochrany Drevárska fakulta, Technická univerzita vo Zvolene
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Nuclear Astrophysics II Lecture 5 Fri. June 1, 2012 Prof. Shawn Bishop, Office 2013, Ex. 12437
[email protected]
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Lecture 15 Explosive Nucleosynthesis and the r-Process
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1 AGB - Asymptotic Giant Branch wykład II Ryszard Szczerba Centrum Astronomiczne im. M. Kopernika, Toruń
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(56) 62 19 249 ext. 27
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Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth
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Townsley and L. B., 2004, Ap. J., 600, 390 (Theoretical overview)
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