標題: Titlebook: Chemical Evolution of Galaxies; Francesca Matteucci Book 2012 Springer-Verlag Berlin Heidelberg 2012 Chemical Evolution of Galaxies.Classi [打印本頁] 作者: mentor 時間: 2025-3-21 18:59
書目名稱Chemical Evolution of Galaxies影響因子(影響力)
書目名稱Chemical Evolution of Galaxies影響因子(影響力)學科排名
書目名稱Chemical Evolution of Galaxies網(wǎng)絡(luò)公開度
書目名稱Chemical Evolution of Galaxies網(wǎng)絡(luò)公開度學科排名
書目名稱Chemical Evolution of Galaxies被引頻次
書目名稱Chemical Evolution of Galaxies被引頻次學科排名
書目名稱Chemical Evolution of Galaxies年度引用
書目名稱Chemical Evolution of Galaxies年度引用學科排名
書目名稱Chemical Evolution of Galaxies讀者反饋
書目名稱Chemical Evolution of Galaxies讀者反饋學科排名
作者: 友好 時間: 2025-3-21 23:40 作者: 帶子 時間: 2025-3-22 03:07
Simple Models of Chemical Evolution,r the . (IRA), which states that all stars less massive than or equal to 1.. live forever, while all stars more massive than 1.. die instantaneously. This approximation is correct for stars below 1.. but it is incorrect for larger masses with lifetimes not negligible relative to the age of the Unive作者: 劇本 時間: 2025-3-22 05:55 作者: Feigned 時間: 2025-3-22 11:52 作者: progestin 時間: 2025-3-22 14:50 作者: progestin 時間: 2025-3-22 19:53
Chemical Evolution of Irregular Galaxies,nd rather simple objects with low metallicity and large gas content, suggesting that they are either young objects or have undergone discontinuous star formation activity (bursts) or a continuous but not efficient star formation. They are very interesting objects for studying galaxy evolution: in fa作者: 草本植物 時間: 2025-3-22 22:32 作者: 朝圣者 時間: 2025-3-23 05:10 作者: larder 時間: 2025-3-23 06:08
Francesca MatteucciEducates graduate students and young researchers to start their own research in the field.Outlines theoretical models of chemical evolution of galaxies and compares them with observational results.Tre作者: oxidant 時間: 2025-3-23 11:08
Astronomy and Astrophysics Libraryhttp://image.papertrans.cn/c/image/224335.jpg作者: 思想靈活 時間: 2025-3-23 15:18
Problem Solving Questions in Toxicology:nts, such as hydrogen (H), deuterium (D), helium (He), and a very tiny fraction of lithium (.Li) were formed, while all the other elements from carbon to uranium and beyond were formed inside the stars. The chemical elements and their isotopes are characterized by their mass number (.), namely, the 作者: instill 時間: 2025-3-23 18:50
https://doi.org/10.1007/978-3-030-50409-0history or stellar birthrate function, the stellar yields (nucleosynthesis), and gas flows will be discussed. The most common recipes adopted in the literature for these ingredients will be summarized together with the related uncertainties. Relative to the stellar yields, we will present the nucleo作者: 低三下四之人 時間: 2025-3-24 01:00
Problem Solving Questions in Toxicology:r the . (IRA), which states that all stars less massive than or equal to 1.. live forever, while all stars more massive than 1.. die instantaneously. This approximation is correct for stars below 1.. but it is incorrect for larger masses with lifetimes not negligible relative to the age of the Unive作者: pacifist 時間: 2025-3-24 03:46
Problem Solving Questions in Toxicology: are discussed, such as the star formation rate, the initial mass function, the SN rates, the infall, radial flow, and wind rates. The importance of taking into account the stellar lifetimes together with a critical discussion on the errors on such lifetimes are highlighted. Particular importance is作者: 印第安人 時間: 2025-3-24 09:53
Problem Solving Questions in Toxicology:e bulge, the thick, and the thin disk will be described. Comparison between model results and observations, concerning abundance patterns in the stars of the different Galactic components and radial gradients along the thin disk, can suggest to us the main mechanisms for the formation of our Galaxy.作者: 恫嚇 時間: 2025-3-24 11:16 作者: OTTER 時間: 2025-3-24 18:09
A Historical Glimpse and Stalwartsnd rather simple objects with low metallicity and large gas content, suggesting that they are either young objects or have undergone discontinuous star formation activity (bursts) or a continuous but not efficient star formation. They are very interesting objects for studying galaxy evolution: in fa作者: 光明正大 時間: 2025-3-24 22:14 作者: irradicable 時間: 2025-3-25 02:57 作者: Confidential 時間: 2025-3-25 03:22
978-3-642-43005-3Springer-Verlag Berlin Heidelberg 2012作者: 舊石器 時間: 2025-3-25 08:48
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作者: 褪色 時間: 2025-3-25 12:20
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作者: 大火 時間: 2025-3-25 18:01
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.作者: Toxoid-Vaccines 時間: 2025-3-25 20:02 作者: 災(zāi)禍 時間: 2025-3-26 03:31
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.作者: 實施生效 時間: 2025-3-26 08:16 作者: Occupation 時間: 2025-3-26 11:10 作者: 希望 時間: 2025-3-26 16:07 作者: IRS 時間: 2025-3-26 18:38 作者: Antimicrobial 時間: 2025-3-26 23:11
A Historical Glimpse and Stalwartslar galaxies could also be important contributors to the population of systems giving rise to QSO-absorption lines at high redshift, in particular the damped-Lyman-α systems.In this chapter, we also show the mass–metallicity relation found for star forming galaxies at low and high redshift and discuss some possible interpretations.作者: 向外供接觸 時間: 2025-3-27 03:58
Simple Models of Chemical Evolution, need to be made. We show first the solution of the . and then more complex solutions for cases with galactic flows such as outflow, infall, and radial inflow. We also show the failure of analytical models in reproducing the observations.作者: Finasteride 時間: 2025-3-27 06:52 作者: innovation 時間: 2025-3-27 12:00
Chemical Evolution of Early Type Galaxies, stellar populations are derived. The evolution of ellipticals hosting quasars is discussed. The properties of dwarf spheroidal galaxies in the local group are discussed, and by comparing the predicted and observed abundances, we try to understand whether they could have been the building blocks of the Milky Way.作者: Modify 時間: 2025-3-27 15:35 作者: 變形詞 時間: 2025-3-27 21:30 作者: 兩種語言 時間: 2025-3-27 22:44 作者: NEX 時間: 2025-3-28 02:49
Introduction, some .Li during spallation processes, which derive from the interaction between cosmic rays and interstellar atoms of carbon (C), nitrogen (N), and oxygen (O). All the elements with . ≥ 12 starting from .C have been synthesized inside the stars and the sum of all of them in Astronomy is called . and indicated with capital ..作者: Boycott 時間: 2025-3-28 06:18
Chemical Evolution of the Milky Way and Other Spirals, more detail. Observational data on spiral galaxies suggest that there has been a downsizing in the star formation, in the sense that the most massive spirals should have formed more quickly and with a more efficient star formation than the less massive ones, and therefore they should be older.作者: 良心 時間: 2025-3-28 13:14 作者: 教唆 時間: 2025-3-28 14:52 作者: badinage 時間: 2025-3-28 21:07
10樓作者: 死貓他燒焦 時間: 2025-3-29 00:12
10樓
