Cubicle 发表于 2025-3-25 06:33:37

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辩论的终结 发表于 2025-3-25 07:44:14

High-Redshift Galaxies978-3-540-75824-2Series ISSN 0941-7834 Series E-ISSN 2196-9698

resistant 发表于 2025-3-25 15:05:34

Basic Techniques and their Limitationselativistic particles. Neutrinos and gravitational waves propagate like light rays. But the low sensitivity of the corresponding detectors makes it impossible to observe high-redshift sources of neutrinos and gravitational waves.

善辩 发表于 2025-3-25 16:52:44

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共栖 发表于 2025-3-25 19:58:57

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Neonatal 发表于 2025-3-26 01:47:08

The Past and the Futurewas transparent to light. Fortunately this was the case during more than 99.99% of the age of the universe. Only during the first about 380 000 years (corresponding to redshifts . > 1090) the expanding universe was (due to the high free-electron density) opaque to light of all wavelengths.

Iniquitous 发表于 2025-3-26 06:56:46

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capsule 发表于 2025-3-26 08:39:50

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文件夹 发表于 2025-3-26 12:54:13

0941-7834 cientific results on high-redshift galaxies accumulated duriThe high-redshift galaxies became a distinct research ?eld during the ?nal decade of the20thcentury. AtthattimetheLyman-breaktechniquemadeitpossibletoidentify signi?cant samples of such objects, and the new generation of 8 to 10-m telescope

Cpap155 发表于 2025-3-26 18:53:23

Book 20091st editionidentify signi?cant samples of such objects, and the new generation of 8 to 10-m telescopes resulted in ?rst good spectroscopic data. Today the high-redshift galaxies have developed into one of the important topics of astrophysics, accounting for about 5–10% of the publications in the major scienti?
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查看完整版本: Titlebook: High-Redshift Galaxies; Light from the Early Immo Appenzeller Book 20091st edition Springer-Verlag Berlin Heidelberg 2009 Cosmology.Dark En