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Titlebook: Chemical Evolution of Galaxies; Francesca Matteucci Book 2012 Springer-Verlag Berlin Heidelberg 2012 Chemical Evolution of Galaxies.Classi

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21#
發(fā)表于 2025-3-25 03:22:39 | 只看該作者
978-3-642-43005-3Springer-Verlag Berlin Heidelberg 2012
22#
發(fā)表于 2025-3-25 08:48:53 | 只看該作者
Book 2012curring in stars and to gas flows into and out of galaxies. .This book deals with the chemical evolution of galaxies of all morphological types (ellipticals, spirals and irregulars) and stresses the importance of the star formation histories in determining the properties of stellar populations in di
23#
發(fā)表于 2025-3-25 12:20:20 | 只看該作者
0941-7834 of galaxies and compares them with observational results.Tre.The term “chemical evolution of galaxies” refers to the evolution of abundances of chemical species in galaxies, which is due to nuclear processes occurring in stars and to gas flows into and out of galaxies. .This book deals with the chem
24#
發(fā)表于 2025-3-25 18:01:59 | 只看該作者
https://doi.org/10.1007/978-3-030-50409-0iterature for these ingredients will be summarized together with the related uncertainties. Relative to the stellar yields, we will present the nucleosynthesis calculations for stars of all masses, together with the most recent ideas about supernova (II, I) progenitors. The importance of gas flows and their observational evidence will be reviewed.
25#
發(fā)表于 2025-3-25 20:02:15 | 只看該作者
26#
發(fā)表于 2025-3-26 03:31:25 | 只看該作者
Basic Ingredients for Modeling Chemical Evolution,iterature for these ingredients will be summarized together with the related uncertainties. Relative to the stellar yields, we will present the nucleosynthesis calculations for stars of all masses, together with the most recent ideas about supernova (II, I) progenitors. The importance of gas flows and their observational evidence will be reviewed.
27#
發(fā)表于 2025-3-26 08:16:28 | 只看該作者
28#
發(fā)表于 2025-3-26 11:10:23 | 只看該作者
29#
發(fā)表于 2025-3-26 16:07:13 | 只看該作者
30#
發(fā)表于 2025-3-26 18:38:16 | 只看該作者
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