標(biāo)題: Titlebook: Galaxy Formation; Malcolm S. Longair Textbook 2023Latest edition The Editor(s) (if applicable) and The Author(s), under exclusive license [打印本頁] 作者: Johnson 時間: 2025-3-21 17:39
書目名稱Galaxy Formation影響因子(影響力)
書目名稱Galaxy Formation影響因子(影響力)學(xué)科排名
書目名稱Galaxy Formation網(wǎng)絡(luò)公開度
書目名稱Galaxy Formation網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Galaxy Formation被引頻次
書目名稱Galaxy Formation被引頻次學(xué)科排名
書目名稱Galaxy Formation年度引用
書目名稱Galaxy Formation年度引用學(xué)科排名
書目名稱Galaxy Formation讀者反饋
書目名稱Galaxy Formation讀者反饋學(xué)科排名
作者: 不安 時間: 2025-3-22 00:15
The Large Scale Structure of the Universeion (CMB) over the sky and its spectrum. The remarkable isotropy of the CMB contrasts with large-scale distribution of galaxies which display huge walls and voids on large scales, which has a sponge-like topology. Their distributions are described by correlation functions. Combining Hubble’s law wit作者: Disk199 時間: 2025-3-22 03:53
Galaxies, interacting, starburst and active galaxies. Correlations among the populations of galaxies include the red and blue sequences, colour versus absolute magnitude, the light distribution in galaxies and the Sérsic Index. Correlations among their spectroscopic and gaseous properties include mean stell作者: 北極人 時間: 2025-3-22 07:42 作者: Filibuster 時間: 2025-3-22 09:00
The Theoretical Frameworkrelating observables to the intrinsic properties of the objects studied. The application of the cosmological principle and the development of the metric for isotropic curved spaces leads to the Robertson-Walker metric. This metric provides the tool for understanding the significance of the cosmologi作者: 藝術(shù) 時間: 2025-3-22 14:07
An Introduction to Relativistic Gravityprovides insights into how it differs from Newtonian gravity. The theory is based upon the Principle of Equivalence which leads to the gravitational redshift and the bending of light rays in curved space-time. Detailed tests of the theory involve Parameterised Post-Newtonian (PPN) models for the fou作者: 藝術(shù) 時間: 2025-3-22 19:21 作者: 擔(dān)憂 時間: 2025-3-22 21:51
The Determination of Cosmological Parametersot the predictions of the models are in accord with observations of the extragalactic Universe. First, we parameterise the predictions of the models with quantities we might hope to measure. The classical cosmological tests in which standard properties galaxies and other extragalactic objects are de作者: 排他 時間: 2025-3-23 01:56 作者: Legend 時間: 2025-3-23 05:31
Nucleosynthesis in the Early Universelving the problem of the present day abundances of the light elements. First, we need to establish the equilibrium abundances of all species which contribute to the inertial mass density of the Universe and how it changes with cosmic epoch. This involves understanding how weakly interacting particle作者: 取回 時間: 2025-3-23 11:40 作者: Parallel 時間: 2025-3-23 16:51
More Tools and Problemsls to be confronted with observation. We first need the concept of the horizon scales which are present in expanding world models and their physical significance. These are developed for the critical world model, Ω.?=?1, Ω.?=?0 and then for the preferred reference model Ω.?=?0.3, Ω.?=?0.7. This lead作者: 旅行路線 時間: 2025-3-23 21:50
Dark Matter and Galaxy Formationnd cosmology. Possible forms of non-baryonic dark matter are reviewed, including massive neutrinos, axions and WIMPS. Broadly, the models can be classified under the generic terms Hot and Cold Dark Matter scenarios. Important themes include the free-streaming of ultra-weakly interacting particles an作者: invade 時間: 2025-3-24 00:56 作者: Cholesterol 時間: 2025-3-24 04:07 作者: 走路左晃右晃 時間: 2025-3-24 07:25 作者: Debrief 時間: 2025-3-24 11:53
Biomechanics of Flexor Pulley Reconstructionion (CMB) over the sky and its spectrum. The remarkable isotropy of the CMB contrasts with large-scale distribution of galaxies which display huge walls and voids on large scales, which has a sponge-like topology. Their distributions are described by correlation functions. Combining Hubble’s law wit作者: 驚奇 時間: 2025-3-24 16:04
Theodore V. Hromadka II,Robert J. Whitley, interacting, starburst and active galaxies. Correlations among the populations of galaxies include the red and blue sequences, colour versus absolute magnitude, the light distribution in galaxies and the Sérsic Index. Correlations among their spectroscopic and gaseous properties include mean stell作者: 粗鄙的人 時間: 2025-3-24 20:19 作者: 王得到 時間: 2025-3-25 00:29
P. A. Muraro,A. Lugaresi,D. Gambirelating observables to the intrinsic properties of the objects studied. The application of the cosmological principle and the development of the metric for isotropic curved spaces leads to the Robertson-Walker metric. This metric provides the tool for understanding the significance of the cosmologi作者: 拾落穗 時間: 2025-3-25 07:20 作者: 猛擊 時間: 2025-3-25 08:06
Barry M. Freifeld,Timothy J. Kneafseyo and non-zero. A helpful Newtonian analogue is discussed. There follows a detailed analysis of the dynamics of the Friedman models and of the relation between intrinsic properties and observables. Density parameters for baryonic, dark matter and the dark energy are introduced. The relations between作者: DAFT 時間: 2025-3-25 13:10 作者: Highbrow 時間: 2025-3-25 18:13 作者: overhaul 時間: 2025-3-25 22:16 作者: 鞭打 時間: 2025-3-26 01:14
Advances on Robotic Item Pickinge basic physics of gravitational collapse is built up, starting with the non-relativistic case and the Jeans’ instability. Gravitational collapse in a static and expanding medium is contrasted—exponential growth of the instability in the case of a static medium and algebraic collapse in an expanding作者: Unsaturated-Fat 時間: 2025-3-26 08:12 作者: ablate 時間: 2025-3-26 11:32
https://doi.org/10.1007/978-3-319-53487-9nd cosmology. Possible forms of non-baryonic dark matter are reviewed, including massive neutrinos, axions and WIMPS. Broadly, the models can be classified under the generic terms Hot and Cold Dark Matter scenarios. Important themes include the free-streaming of ultra-weakly interacting particles an作者: 充滿裝飾 時間: 2025-3-26 12:38 作者: inconceivable 時間: 2025-3-26 19:49 作者: forthy 時間: 2025-3-26 21:26
978-3-662-65893-2The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer-Verlag GmbH, DE作者: COKE 時間: 2025-3-27 02:20 作者: 意外 時間: 2025-3-27 06:14
Malcolm S. LongairDiscusses the fundamental physics behind the recent developments in astrophysical cosmology.A very widely appreciated text highlighting the fundamentals of the current ‘best-buy’ model of the Universe作者: 秘密會議 時間: 2025-3-27 09:34 作者: Agronomy 時間: 2025-3-27 15:11
Textbook 2023Latest editions of Type 1a supernovae and many other remarkable recent observations..This book serves as an ideal text for graduate level courses on astrophysical cosmology and is also highly appreciated as a reference source for professional astrophysicist and cosmologists..作者: AORTA 時間: 2025-3-27 21:14 作者: 群島 時間: 2025-3-28 01:54
Theodore V. Hromadka II,Robert J. Whitley a remarkably uniform shape, although the brightest galaxies in clusters are special cases. The luminosity functions for different classes of galaxy depend upon the galaxy environment. Mean mass-to-luminosity ratios for visible matter in the Universe are determined.作者: MOAT 時間: 2025-3-28 04:20 作者: 遭受 時間: 2025-3-28 07:53 作者: Stress 時間: 2025-3-28 13:30 作者: IVORY 時間: 2025-3-28 14:57
A Very Brief History of Cosmology and Galaxy Formationarameters, in agreement with observations in other wavebands. These understandings lead to problems which may be resolved by studies of the very early Universe. These topics are discussed in detail in the succeeding chapters.作者: Microaneurysm 時間: 2025-3-28 22:37
Galaxies a remarkably uniform shape, although the brightest galaxies in clusters are special cases. The luminosity functions for different classes of galaxy depend upon the galaxy environment. Mean mass-to-luminosity ratios for visible matter in the Universe are determined.作者: miracle 時間: 2025-3-29 02:27
The Determination of Cosmological Parametersl lenses and estimates of the density parameter Ω.. The current status and issues involved in these approaches are reviewed. A second complementary and independent approach involves studies of the CMB, both for understanding the origin of the light elements and its consequences for determining the b作者: 使更活躍 時間: 2025-3-29 03:15 作者: 遭受 時間: 2025-3-29 10:22
The Cosmic Microwave Background Radiationhe whole analysis, including the determination of the cosmological parameters can be carried out entirely from analysis of the CMB data-sets. The values found are consistent with those determined by independent approaches.作者: 金哥占卜者 時間: 2025-3-29 15:00
0941-7834 an ideal text for graduate level courses on astrophysical cosmology and is also highly appreciated as a reference source for professional astrophysicist and cosmologists..978-3-662-65893-2978-3-662-65891-8Series ISSN 0941-7834 Series E-ISSN 2196-9698 作者: Rejuvenate 時間: 2025-3-29 19:06 作者: phlegm 時間: 2025-3-29 22:46
Biomechanics of Flexor Pulley Reconstructionls and voids on large scales, which has a sponge-like topology. Their distributions are described by correlation functions. Combining Hubble’s law with the isotropy and homogeneity of the Universe shows that the Universe as a whole is expanding uniformly.作者: 猜忌 時間: 2025-3-30 01:12
https://doi.org/10.1007/978-3-319-53487-9ified under the generic terms Hot and Cold Dark Matter scenarios. Important themes include the free-streaming of ultra-weakly interacting particles and gravitational instabilities in the presence of dark matter. These considerations lead to scenarios for the formation of structure in Hot and Cold Dark Matter models.作者: Ossification 時間: 2025-3-30 06:13
Rubens Gon?alves Salsa Junior,Fai Mad from the electromagnetic Universe, extrapolating as far back into the early Universe as laboratory physics will allow. The key concept of the variation of the speed of sound with cosmic epoch is given a preliminary hearing.作者: moribund 時間: 2025-3-30 10:48 作者: chronicle 時間: 2025-3-30 16:12
