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

爆裂

書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record影響因子(影響力)




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record影響因子(影響力)學(xué)科排名




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record被引頻次




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record被引頻次學(xué)科排名




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record年度引用




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record年度引用學(xué)科排名




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record讀者反饋




書(shū)目名稱Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record讀者反饋學(xué)科排名

Interdict

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

Panacea

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

憤慨點(diǎn)吧

Cytokines

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

責(zé)怪

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

責(zé)怪

fallible

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

刻苦讀書(shū)

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

集合