Titlebook: Observational Cosmology; Proceedings of the 1 Adelaide Hewitt,Geoffrey Burbidge,Li Zhi Fang Conference proceedings 1987 International Astro

會(huì)議記錄

書(shū)目名稱Observational Cosmology影響因子(影響力)




書(shū)目名稱Observational Cosmology影響因子(影響力)學(xué)科排名




書(shū)目名稱Observational Cosmology網(wǎng)絡(luò)公開(kāi)度




書(shū)目名稱Observational Cosmology網(wǎng)絡(luò)公開(kāi)度學(xué)科排名




書(shū)目名稱Observational Cosmology被引頻次




書(shū)目名稱Observational Cosmology被引頻次學(xué)科排名




書(shū)目名稱Observational Cosmology年度引用




書(shū)目名稱Observational Cosmology年度引用學(xué)科排名




書(shū)目名稱Observational Cosmology讀者反饋




書(shū)目名稱Observational Cosmology讀者反饋學(xué)科排名

不如屎殼郎

Primordial Nucleosynthesis of 7Lit exception between the atmospheric Li/H ratio and Te, and (2) at Te and (2) at T ≤ 5600 K the average lithium abundance is

= 1.2 ± 0.3 x .. The latter value constitutes a lower limit on the ^Li fraction produced in primordial nucleosynthesis and thereby significantly constrains the cosmic ratio of baryons to photons.

jealousy

commonsense

Observational Cosmology 1920–1985: An Introduction to the Conferenceed as they have been discussed in the archive literature. The problem of observational bias is emphasized, as is the difficult recent search for secular evolutionary effects. Current problems which have prospects for solutions in the next decades are set out in the final section.

abduction

Debark

1743-9213 he observational aspects of modern cosmology was taken in part because this conference has come in a period when there have been several international meetings on one aspect of modern cosmology, namely the early universe and its possible relationship to particle physics. While that approach is extre

施魔法

The Status of the Hubble Diagram In 1986volution effects, which dominate over the cosmological model differences. Most radio galaxies apparently have had active star formation, with a continually declining rate, but a few are quite faint and red; they may have had a relatively passive evolution.

極端的正確性

exclamation

The Cosmic Microwave Backgroundcale angular distribution are described, as well as searches for small angular scale fluctuations on arcsecond to degree scales. A few of the consequences of these measurements and upper limits for cosmology, astrophysics, and theories of galaxy formation are touched on here.

使絕緣

High Sensitivity Observations of the Microwave Background Radiationevolves into the present-day Universe (z = 0). Such measurements provide stringent tests of the cosmological theories of universal evolution and have implications for allowed values of the density and composition of matter in the Universe.