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Titlebook: Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record; Proceedings of a Col M. Spite Conference proceedings 1999 S

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发表于 2025-3-21 16:46:20 | 显示全部楼层 |阅读模式
书目名称Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record
副标题Proceedings of a Col
编辑M. Spite
视频video
图书封面Titlebook: Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record; Proceedings of a Col M. Spite Conference proceedings 1999 S
描述This book contains the Proceedings of the first ‘Rencontres de l‘Observatoire‘ which was held at the Meudon campus of the Paris Observatory on September 21-25, 1998. The subject addressed was ‘Galaxy evolution: Connecting the distant Universe with the local fossil record‘. This colloquium was a project devised by a group of astronomers who, in France but also in Europe, in the United States, in South America, and even in Japan, have worked for a long time with Roger and Giusa Cayrel. Roger and Giusa had a tremendous influence on us all. They taught us in their discrete way, the care of the observations and the rigor in the interpretation. Besides the presentations of Jun Jugaku and Rene Racine and the presentation of Pierre Couturier of the story of the Canada-France-Hawaii Telescope (presentation which unfortunately does not appear in this book) several papers refer to the role of Roger and Giusa in astronomy. Their contribution to the study of the galactic evolution has been fundamental. Our Milky Way is the galaxy which can be studied in most details. From the study of our Galaxy‘s old population, one can understand what our Milky Way was like very soon after its birth, at the s
出版日期Conference proceedings 1999
关键词Bulge; Galaxy; Population; Universe; astronomy; astrophysics; milky way; observational astronomy
版次1
doihttps://doi.org/10.1007/978-94-011-4213-7
isbn_softcover978-94-010-5831-5
isbn_ebook978-94-011-4213-7
copyrightSpringer Science+Business Media Dordrecht 1999
The information of publication is updating

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发表于 2025-3-21 21:43:07 | 显示全部楼层
Primordial Nucleosynthesisgst the first astronomers I have met here in Paris when I arrived more than 30 years ago. (I already knew the astronomical papers of Roger during my previous stay at The Institute for Space Studies in New York). I will always remember their warm family welcome. With their charming little girls (Fran
发表于 2025-3-22 03:24:57 | 显示全部楼层
Deuterium, Lithium and the Density of the Universeuclear density parameter Ω.. The relative advantages/disadvantages of D and .Li as the proper ‘baryometer’ are discussed. In favour of D, the main arguments are the relative simplicity of the formation/destruction schema, but this is challenged by the large uncertainties on the choice of its actual
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New Insights into the Early Stage of the Galactic Chemical Evolutionitor main-sequence stars .. from the abundance patterns of extremely metal-poor stars with a procedure recently proposed by Shigeyama and Tsujimoto (1998). The yields thus obtained are indispensable because theoretical SN II models to date can reliably predict the amounts of only a few elements. The
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Stellar Evolution and the Cosmologial Supernovae RatesN Ia are considered. We compute the cosmic rate histories for SN I, SN II and both classes of SN Ia, and present them in the form of redshift and magnitude distributions. These results can be compared with observational data, allowing to estimate the star formation rate history and the cosmological
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Observing Boron in Metal-Poor Starselected according to the availability (in the literature) of their lithium and beryllium abundances, because the simultaneous knowledge of LiBeB in the same targets is a powerful diagnostic for testing depletion and internal mixing predicted by different stellar structure models. Two stars (HD 94028
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Li Be B Energetics and Cosmic Ray Origin solar composition scaled with metallicity; the CRS model in which cosmic rays with composition similar to that of the current epoch cosmic rays are accelerated out of fresh supernova ejecta; and the LECR model in which a distinct low energy component coexists with the postulated cosmic rays of the
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