標題: Titlebook: Confrontation of Cosmological Theories with Observational Data; M. S. Longair Book 1974 The International Astronomical Union 1974 Big Bang [打印本頁] 作者: 五個 時間: 2025-3-21 18:57
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作者: BYRE 時間: 2025-3-21 21:35
Confrontation of Lema?tre Models and the Cosmological Constant with Observationsmological constant if non-zero must be in absolute value less than 2 × 10. cm.. The predictions of the Lema?tre models are compared with modern observations. It is shown that Lema?tre models without evolution fail to reproduce the observed radio source counts. The existence of quasars with large red作者: Agronomy 時間: 2025-3-22 02:29
The Hubble Constant and the Deceleration Parameterheids, brightest stars, II regions, and luminosity classes) the distance scale is carried beyond any possible local anisotropy of the velocity field. Special care is taken to allow for the dependence of the intrinsic properties of the distance indicators on the size of the parent galaxy, and for the作者: deforestation 時間: 2025-3-22 04:59
Evidence for Non-Velocity Redshiftsin distance, to our own. It is possible that all QSRs originate from galaxies of much lower redshift. It is shown that in the four cases where QSRs fall projected closest to bright galaxies, that in all four cases the galaxies show evidence of physical interaction. Evidence for high redshift, compac作者: Fracture 時間: 2025-3-22 09:26 作者: 否決 時間: 2025-3-22 13:18
The Counts of Radio Sourceses, we must look at . the counts of radio sources at . frequencies; second, when we attempt to evaluate the implications of the source counts, we should use proper cosmological models and not rely on the local Euclidean model.作者: 否決 時間: 2025-3-22 17:18
Radio Source Counts at Centimetre Wavelengthsppear to differ markedly from an integral number-flux relation having a slope of ?1.5 between 5 and 5 × 10. sources per steradian, and show a sharp drop at source densities smaller then 5 sr.. On the basis of the form of the number counts and the observed anisotropies in the distribution of sources 作者: TRAWL 時間: 2025-3-23 00:29
Observational Foundations of Inhomogeneous Universealysed..The results of the analysis show that there is a significant non-random surface distribution of galaxies irrespective of the scale of the field investigated. The observed clumpiness does not allow us to introduce discrete hierarchical structures. The distribution of galaxies shows rather a c作者: FLAX 時間: 2025-3-23 02:24
Field Galaxies and Cluster Galaxies: Abundances of Morphological Types and Corresponding Luminosity of selection probabilities, and (iii) of ‘space luminosity functions’. Strictly, the theory applies to ‘homogeneous classes’ of galaxies. This term designates a category of galaxies, say ., so finely defined that the probability, say .(. | .), that a galaxy of category . will be included in the cata作者: 離開真充足 時間: 2025-3-23 09:16
Large Scale Anisotropy of the Cosmic Microwave Background origin. Measurements of the spectrum of the radiation, discussed earlier in this volume by Blair, are consistent with the idea that the radiation is in fact a relic of a hot, dense, initial state of the Universe — the Big Bang. If the radiation is cosmological, measurements of both its spectrum and作者: Tempor 時間: 2025-3-23 09:59 作者: Palpitation 時間: 2025-3-23 16:43 作者: 表示問 時間: 2025-3-23 21:43 作者: carotid-bruit 時間: 2025-3-24 01:26 作者: 半導(dǎo)體 時間: 2025-3-24 02:40
International Astronomical Union Symposiahttp://image.papertrans.cn/c/image/235433.jpg作者: 機制 時間: 2025-3-24 09:30 作者: enchant 時間: 2025-3-24 10:53 作者: 勾引 時間: 2025-3-24 17:29 作者: 一起 時間: 2025-3-24 19:07 作者: 公共汽車 時間: 2025-3-24 23:27 作者: 爭議的蘋果 時間: 2025-3-25 06:10 作者: Frisky 時間: 2025-3-25 08:29 作者: 圓柱 時間: 2025-3-25 14:55
https://doi.org/10.1007/978-3-030-79245-9xies from a random one, the cell size dependence of the index of clumpiness, the results of covariance function tests for correlations between different cluster centers and between clusters and individual galaxies, and a power-spectrum analysis. All tests give results that indicate or are compatible作者: Fluctuate 時間: 2025-3-25 15:55
Translating Film Subtitles into Chinesees, we must look at . the counts of radio sources at . frequencies; second, when we attempt to evaluate the implications of the source counts, we should use proper cosmological models and not rely on the local Euclidean model.作者: Extemporize 時間: 2025-3-25 23:39 作者: PLE 時間: 2025-3-26 00:24 作者: notice 時間: 2025-3-26 07:05 作者: 結(jié)果 時間: 2025-3-26 09:30 作者: 神圣將軍 時間: 2025-3-26 15:58 作者: Common-Migraine 時間: 2025-3-26 20:43 作者: Suppository 時間: 2025-3-26 21:11 作者: MEEK 時間: 2025-3-27 01:57 作者: Itinerant 時間: 2025-3-27 05:43
International Criminal Justice SeriesExperimental measurements of the intensity of the submillimeter background are reviewed. The latest results all indicate a low background; it is not yet possible to say whether or not the spectrum in this range is blackbody.作者: 可互換 時間: 2025-3-27 11:55 作者: LAP 時間: 2025-3-27 15:01 作者: Incommensurate 時間: 2025-3-27 18:53
Energy Density of the Relic RadiationExperimental measurements of the intensity of the submillimeter background are reviewed. The latest results all indicate a low background; it is not yet possible to say whether or not the spectrum in this range is blackbody.作者: 推延 時間: 2025-3-28 00:42 作者: 嬰兒 時間: 2025-3-28 04:17
Shifting Trends in International Tribunalsty levels and the number-flux density relations vary from place to place in the GB region and the significance level of the observed variations is at least 1%..The most important conclusion which can be drawn from the GB data is that results obtained from the observations of a single selected region作者: 放縱 時間: 2025-3-28 06:28 作者: 鐵塔等 時間: 2025-3-28 11:55
Confrontation of Cosmological Theories with Observational Data作者: 或者發(fā)神韻 時間: 2025-3-28 16:12
Observational Foundations of Inhomogeneous Universety levels and the number-flux density relations vary from place to place in the GB region and the significance level of the observed variations is at least 1%..The most important conclusion which can be drawn from the GB data is that results obtained from the observations of a single selected region作者: antiquated 時間: 2025-3-28 20:21
Field Galaxies and Cluster Galaxies: Abundances of Morphological Types and Corresponding Luminosity s class..In order to validate the theory empirically, calculations were performed to predict the abundances of eight combinations of morphological types among cluster galaxies listed in the HMS Catalogue, each combination being treated as a distinct homogeneous class. Additional hypotheses underlyin作者: FUME 時間: 2025-3-28 23:56 作者: Odyssey 時間: 2025-3-29 04:50 作者: 拱形面包 時間: 2025-3-29 09:50 作者: Flounder 時間: 2025-3-29 13:01 作者: cylinder 時間: 2025-3-29 15:47 作者: creatine-kinase 時間: 2025-3-29 19:57
The Thermal History of the Universe and the Spectrum of Relic Radiationns of the spectrum of the relic radiation. The absence of noticeable deviations from the Planckian spectrum enables us to set limits to the energy release in the early Universe (10. < z < 10.). But in order to have a clear picture of possible distortions, let us first review the idealized situation.作者: Aids209 時間: 2025-3-29 23:56 作者: 遍及 時間: 2025-3-30 06:09 作者: NATAL 時間: 2025-3-30 11:12 作者: 濃縮 時間: 2025-3-30 16:02 作者: stress-response 時間: 2025-3-30 17:32 作者: mighty 時間: 2025-3-30 20:54
Translating Film Subtitles into Chineses weaker than is generally thought unless the cosmological origin of the quasar redshifts is assumed. Measurements of the radio spectra of the sources suggest a dependence of the spectral curvature on flux density.作者: 燈泡 時間: 2025-3-31 02:46
The Hubble Constant and the Deceleration Parameterof the deceleration constant .. = 1 ±1 was recently derived by Sandage (1972a) and Sandage and Hardy (1973). The most important correction to this value is probably the luminosity evolution of galaxies, which tends to push .. below 0.5. The ensuing evidence for an . is also favored by independent arguments.作者: 沐浴 時間: 2025-3-31 06:01 作者: happiness 時間: 2025-3-31 10:35
Radio Source Counts at Centimetre Wavelengthss weaker than is generally thought unless the cosmological origin of the quasar redshifts is assumed. Measurements of the radio spectra of the sources suggest a dependence of the spectral curvature on flux density.作者: Indicative 時間: 2025-3-31 17:22 作者: 釋放 時間: 2025-3-31 18:47 作者: Melodrama 時間: 2025-3-31 22:36
The Spectrum of Density Perturbations in an Expanding Universeation at z~1000 and provide the primordial fluctuations that can eventually generate galaxies. A closely related matter, that of the associated fluctuations in the background radiation, is discussed elsewhere in this volume by Doroshkevich, Sunyaev and Zel’dovich.作者: 敬禮 時間: 2025-4-1 03:57
On Leadership, Followership, and Cultureith a different group of followers. Moreover, most writers agree that leadership can be taught and learned, even though others believe that certain leadership talents are inborn. This is an ongoing debate that we shall certainly address.
