GALACTIC GLOBULAR CLUSTERS: IDEAL LABORATORIES TO TEST STELLAR NUCLEOSYNTHESIS?
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- EAS Publications Series, 2008, v. 32, p. 369, doi. 10.1051/eas:0832011
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Works matching IS 16334760 AND DT 2008 AND VI 32
Results: 12
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ABUNDANCES IN THE MOST METAL-POOR STARS: NUCLEOSYNTHESIS IN THE EARLY MILKY WAY.
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- EAS Publications Series, 2008, v. 32, p. 357, doi. 10.1051/eas:0832010
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- Article
3
AN INTRODUCTION TO GALACTIC CHEMICAL EVOLUTION.
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- EAS Publications Series, 2008, v. 32, p. 311, doi. 10.1051/eas:0832009
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- Article
4
TYPE IA SUPERNOVAE.
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- EAS Publications Series, 2008, v. 32, p. 283, doi. 10.1051/eas:0832008
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- Article
5
FINAL STAGES OF MASSIVE STARS. SN EXPLOSION AND EXPLOSIVE NUCLEOSYNTHESIS.
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- EAS Publications Series, 2008, v. 32, p. 233, doi. 10.1051/eas:0832007
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- Article
6
NUCLEOSYNTHESIS FROM MASSIVE STARS 50 YEARS AFTER B<sup>2</sup>FH.
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- EAS Publications Series, 2008, v. 32, p. 187, doi. 10.1051/eas:0832006
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- Article
7
PLANETARY NEBULAE, TRACERS OF STELLAR NUCLEOSYNTHESIS.
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- EAS Publications Series, 2008, v. 32, p. 173, doi. 10.1051/eas:0832005
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- Article
8
STRUCTURAL AND CHEMICAL EVOLUTION OF LOWAND INTERMEDIATE-MASS STARS.
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- EAS Publications Series, 2008, v. 32, p. 131, doi. 10.1051/eas:0832004
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- Article
9
TRANSPORT PROCESSES IN STARS: DIFFUSION, ROTATION, MAGNETIC FIELDS AND INTERNAL WAVES.
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- EAS Publications Series, 2008, v. 32, p. 81, doi. 10.1051/eas:0832003
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- Article
10
AN INTRODUCTION TO PRIMORDIAL NUCLEOSYNTHESIS.
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- EAS Publications Series, 2008, v. 32, p. 61, doi. 10.1051/eas:0832002
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11
THE NUCLEAR PHYSICS INPUT TO ASTROPHYSICS MODELLING, AND THE R- AND P-PROCESSES: WHERE DO WE STAND 50 YEARS AFTER B<sup>2</sup>FH AND CAMERON?
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- EAS Publications Series, 2008, v. 32, p. 1, doi. 10.1051/eas:0832001
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12
Foreword.
- Published in:
- EAS Publications Series, 2008, v. 32, p. 1, doi. 10.1051/eas:0832000
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