著者紹介

内容

目次

1. Introduction; 2. Cosmological nucleosynthesis; 3. Primordialnucleosynthesis; 4. Baryon inhomogeneous cosmologies and primordialnucleosynthesis of Li-Be-B; 5. The primordial abundancies of Li and Be; 6. Liand O in stellar populations of our galaxy; 7. Signatures of inhomogeneity inthe early universe; 8. Nuclear data relevant to nucleosynthesis; 9. Theoriesof element synthesis in supernovae; 10. Nucleosynthesis in type I and II SN;11. Nucleosynthesis in SNe II and a function of progenitor mass; 12. On the(O/Fe) vs (Fe/H) relationship at low metallicity; 13. Primordial lithiumabundance from observations of SN 1987A; 14. Stellar opacities; 15. Data forabsorption line analysis; 16. Precision spectroscopy and stellar parametersfrom absorption line systems; 17. Stellar abundance methods; 18.Observational effects of nucleosynthesis in evolved stars; 19. Updating solarabundances; 20. Abundance distribution in galactic stellar populations; 21.Stellar populations in other galaxies; 22. Abundancies, star formation andnuclear activity in galaxies; 23. Global heating of the ionized gas inNGC1068; 24. Observed nuclear abundance effects in Planetary nebulae; 25.Abundances in planetary nebulae in the magellanic clouds and galactic halo;26. N/O ratios in planetary nebulae and central star masses; 27. Latedecaying particles and the ionization of HI regions; 28. Photo-ionizationmodels; 29. Observations of the NII 122 microns line; 30 Nebular abundancesand the chemical evolution of galaxies; 31. Chemical evolution in nearbygalaxies; 32. The most metal poor stars; 33. The mass-metallicity relation;34. Extremely low metallicity galaxies; 35. Chemical evolution of high zgalaxies; 36. S-process abundances in metal poor stars; 37. The chemicalevolution of the light S-elements: yields from massive stars; 38. Abundancedistribution in galactic stellar populations; 39. Abundance gradients in diskgalaxies; 40. A diatribe on the chemical evolution of galaxies; 41. Chemicaland dynamical evolution of galactic disks; 42. The interstellar medium athigh and low redshifts; 43. Abundances in interstellar gas in galaxies in thefield of QSOs; 44. QSO absorption line absorbers; 45. Metallicitymeasurements beyond z=o.3; 46. Resume.