標(biāo)題: Titlebook: Clusters and Superclusters of Galaxies; A. C. Fabian Book 1992 Springer Science+Business Media Dordrecht 1992 Galaxy.Gravity.Quasar.Univer [打印本頁(yè)] 作者: 爆發(fā) 時(shí)間: 2025-3-21 17:40
書(shū)目名稱Clusters and Superclusters of Galaxies影響因子(影響力)
書(shū)目名稱Clusters and Superclusters of Galaxies影響因子(影響力)學(xué)科排名
書(shū)目名稱Clusters and Superclusters of Galaxies網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Clusters and Superclusters of Galaxies網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Clusters and Superclusters of Galaxies被引頻次
書(shū)目名稱Clusters and Superclusters of Galaxies被引頻次學(xué)科排名
書(shū)目名稱Clusters and Superclusters of Galaxies年度引用
書(shū)目名稱Clusters and Superclusters of Galaxies年度引用學(xué)科排名
書(shū)目名稱Clusters and Superclusters of Galaxies讀者反饋
書(shū)目名稱Clusters and Superclusters of Galaxies讀者反饋學(xué)科排名
作者: 生命層 時(shí)間: 2025-3-21 20:51
Far Infrared Emission from Clusters and Warming Flows,red luminosity toward the cD galaxies in rich clusters..Stellar mass loss from galaxies and radiative cooling by dust could produce cool cluster gas at a rate approaching 1000 M./yr unless balanced by a heating mechanism. Thermal electron conduction can be an effective heating agent and we examine w作者: prostate-gland 時(shí)間: 2025-3-22 01:19
The Intracluster Medium,sion processes and physical properties of the ICM are reviewed. The ICM is probably inhomogeneous, with blobs of denser and cooler gas intermixed with hotter, more diffuse gas. If this is correct, the density fluctuations may complicate eft’orts to use the ICM to determine cluster masses and distanc作者: 亞麻制品 時(shí)間: 2025-3-22 05:00
Cooling Flows in Clusters of Galaxies,ations of the ionization state of the optical nebulosity and measurements of Faraday rotation and depolarization of radio lobes show that many luminous radio-loud objects are surrounded by massive cooling flows. They may therefore be an important phase in the formation of the most massive galaxies.作者: 侵略者 時(shí)間: 2025-3-22 11:54 作者: 罵人有污點(diǎn) 時(shí)間: 2025-3-22 15:36
Clusters as Gravitational Lenses, The detection of more than 50 arclets in some rich clusters will enable one to better probe the mass content and the distribution of dark matter in clusters, as well as indications on the redshift distribution of the background galaxies.作者: 罵人有污點(diǎn) 時(shí)間: 2025-3-22 18:19
Superclusters and Large-Scale Structure,erclusters, following recent developments on the scaling properties of galaxies at large separations. Finally, we look at the interplay between galaxy morphology and luminosity on one side, and the supercluster environment (local density) on the other. We discuss recent evidences showing that galaxi作者: 騎師 時(shí)間: 2025-3-22 21:21
Galaxy Clusters Around Quasars, products of this rapid evolution of quasars in rich clusters are radio galaxies in rich clusters at low redshift. By combining data from quasars and low-redshift radio galaxies, it is shown that they can both be consistently described by a single luminosity function and evolution law. Possible expl作者: ESPY 時(shí)間: 2025-3-23 05:06 作者: 抱狗不敢前 時(shí)間: 2025-3-23 09:03
Schwingungen mechanischer Antriebssystemet in many clusters at both optical and X—ray wavelengths. Although its strength and prevalence are hard to quantify, it clearly causes a nmnber of biases both in cluster definition and in the measurement of cluster properties. I illustrate the problems using clusters selected from simulations of a C作者: Instinctive 時(shí)間: 2025-3-23 13:03
https://doi.org/10.1007/978-3-663-05570-9red luminosity toward the cD galaxies in rich clusters..Stellar mass loss from galaxies and radiative cooling by dust could produce cool cluster gas at a rate approaching 1000 M./yr unless balanced by a heating mechanism. Thermal electron conduction can be an effective heating agent and we examine w作者: AIL 時(shí)間: 2025-3-23 14:23 作者: antidepressant 時(shí)間: 2025-3-23 19:07 作者: 小官 時(shí)間: 2025-3-24 00:28
https://doi.org/10.1007/978-3-662-09835-6source required to maintain the ionization of the gas. The physical properties of the nebulae are presented, the difficulties posed by the nebulae for the standard cooling flow scenario are discussed, and possible sources for the origin and ionization of the gas are explored. The evidence points to 作者: condone 時(shí)間: 2025-3-24 05:35 作者: 重疊 時(shí)間: 2025-3-24 09:56
Einfache lineare Schwingungssysteme,erclusters, following recent developments on the scaling properties of galaxies at large separations. Finally, we look at the interplay between galaxy morphology and luminosity on one side, and the supercluster environment (local density) on the other. We discuss recent evidences showing that galaxi作者: Anonymous 時(shí)間: 2025-3-24 14:28
Bodenkr?fte einer Rüttelmaschine products of this rapid evolution of quasars in rich clusters are radio galaxies in rich clusters at low redshift. By combining data from quasars and low-redshift radio galaxies, it is shown that they can both be consistently described by a single luminosity function and evolution law. Possible expl作者: 侵蝕 時(shí)間: 2025-3-24 15:07
Bodenkr?fte einer Rüttelmaschineer epoch by non-gravitational processes. If one discards the optical observations, an alternative is to invoke primordial fluctuations with a much redder spectrum, and I discuss how one might discriminate between these theories with future observations.作者: endocardium 時(shí)間: 2025-3-24 22:26 作者: 推延 時(shí)間: 2025-3-25 02:02 作者: 迅速飛過(guò) 時(shí)間: 2025-3-25 06:17
Imaging the Hot Intracluster Medium,er virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and scale of cluster substructure can be determined.作者: archetype 時(shí)間: 2025-3-25 09:53
Large-Scale Structure within Ten Thousand km/s,d (M) 49, 58, 59, 60, 61, 84, 85, 86, 87, 88, 89, 90 & 91. All these nebulae appear to have no stars. They can be seen only in a very clear sky when they are close to the meridian. Most of these nebulae were given me by M. Mechain”.作者: 親屬 時(shí)間: 2025-3-25 12:23
Clusters and Superclusters of Galaxies978-94-011-2482-9Series ISSN 1389-2185 作者: 原諒 時(shí)間: 2025-3-25 15:54
Zur Synthese von Antriebssystemen,g on the territory of later speakers, I shall limit myself to general and tentative remarks. I shall try to focus on what we can learn about the origin of clusters and superclusters, emphasising that almost all the observations to be discussed at this meeting are relevant to this issue.作者: Generator 時(shí)間: 2025-3-25 20:23 作者: myopia 時(shí)間: 2025-3-26 00:52
Schwingungen mechanischer Antriebssystemeer virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and scale of cluster substructure can be determined.作者: Cougar 時(shí)間: 2025-3-26 08:18 作者: 物質(zhì) 時(shí)間: 2025-3-26 09:10 作者: 中國(guó)紀(jì)念碑 時(shí)間: 2025-3-26 13:23
X-Ray Evolution of Clusters of Galaxies,I review the evidence for the evolution of the X-ray luminosity of clusters of galaxies with cosmic epoch. Such evolution has been found in two independent studies. I discuss the constraints that this evolution places on the primordial density fluctuation spectrum.作者: itinerary 時(shí)間: 2025-3-26 20:18
Nato Science Series C:http://image.papertrans.cn/c/image/228561.jpg作者: 強(qiáng)所 時(shí)間: 2025-3-27 00:54 作者: N防腐劑 時(shí)間: 2025-3-27 04:10
Schwingungen mechanischer Antriebssystemepplying these methods to real optical and X—ray data. The best data sets now give quite precise determinations of the mass in the inner regions of relaxed clusters. The observed ratio of baryonic to total mass in these regions is at least three times larger than that predicted by the standard model 作者: 摻和 時(shí)間: 2025-3-27 09:16
Modellbildung mechanischer Antriebssysteme,ature of these variations and attempts to identify those factors in the galaxies environment which are responsible for them. There is evidence that the environment exerts its effect over the entire history of the galaxy, rather than just at the time of formation, but which of many candidate processe作者: FLORA 時(shí)間: 2025-3-27 10:01
Schwingungen mechanischer Antriebssystemeer virial mass, and the cluster morphology. From these measurements. a lower limit to the baryonic mass in clusters, the formation efficiency of galaxies in different environments, and the presence and scale of cluster substructure can be determined.作者: 侵蝕 時(shí)間: 2025-3-27 17:31 作者: Anthropoid 時(shí)間: 2025-3-27 19:53 作者: attenuate 時(shí)間: 2025-3-27 23:46 作者: Evacuate 時(shí)間: 2025-3-28 03:31
https://doi.org/10.1007/978-3-663-05570-9 rich clusters with cD galaxies, far infrared emission is detected toward the cD galaxy in about 12% of the clusters; the average properties of detections are 〈z〉 = 0.06, 〈L.〉 = 3x10. erg/sec, and 〈T〉 = 25-30 K. This emission probably arises from warm dust heated by electron collisions from the hot 作者: Scintillations 時(shí)間: 2025-3-28 06:59 作者: 眨眼 時(shí)間: 2025-3-28 12:31 作者: MINT 時(shí)間: 2025-3-28 15:16 作者: 有發(fā)明天才 時(shí)間: 2025-3-28 20:16 作者: Orthodontics 時(shí)間: 2025-3-28 22:59 作者: 可互換 時(shí)間: 2025-3-29 03:33 作者: 巧辦法 時(shí)間: 2025-3-29 10:27 作者: 誤傳 時(shí)間: 2025-3-29 12:25 作者: 猛烈責(zé)罵 時(shí)間: 2025-3-29 15:57 作者: 無(wú)辜 時(shí)間: 2025-3-29 23:03
Bodenkr?fte einer Rüttelmaschines massive, but denser and more numerous. The indication from optical searches is that the cluster population is roughly stable in that high velocity dispersion clusters seem to be about as abundant at . ~ 0.5 as at the present while X-ray surveys show a strong negative evolution, there being many fe作者: GRUEL 時(shí)間: 2025-3-30 02:00 作者: companion 時(shí)間: 2025-3-30 06:44
978-94-010-5095-1Springer Science+Business Media Dordrecht 1992作者: 滴注 時(shí)間: 2025-3-30 10:15 作者: 發(fā)微光 時(shí)間: 2025-3-30 16:11 作者: 伴隨而來(lái) 時(shí)間: 2025-3-30 17:28
Rosat Observations of Clusters of Galaxies,h photon yield in the survey like Virgo, Perseus, nad AWM7 are presented to illustrate the capabilities of ROSAT in galaxy cluster studies. In addition we discuss the prospects for detections of clusters of galaxies in the All Sky Survey and their possible implication for cosmological research.作者: anarchist 時(shí)間: 2025-3-31 00:44
,X—Ray Spectral Images of Clusters, spatially resolved spectroscopy and present preliminary BBXRT results on several clusters. The BBXRT results are in good agreement with simple cooling flow theory, in 3 cases confirm the existence of cold material in the cluster, find only shallow abundance gradients and constrain the mass profile in the central regions of the cluster.作者: ELUDE 時(shí)間: 2025-3-31 01:44
,The Sunyaev—Zeldovich Effect,role in elucidating cluster physics, its relationship to other microwave background anisotropies, and the prospects for improved measurements of both its amplitude and two-dimensional structure via a new generation of instruments.作者: 使苦惱 時(shí)間: 2025-3-31 06:45 作者: synchronous 時(shí)間: 2025-3-31 13:11
Book 1992stitute held inCambridge, England in July 1991. .Much of the material is presented in a pedagogical manner and willappeal to scientists, astronomers and graduate students interested inextragalactic astronomy. .作者: aerobic 時(shí)間: 2025-3-31 14:39 作者: CHARM 時(shí)間: 2025-3-31 20:17 作者: 觀察 時(shí)間: 2025-4-1 00:50
Schwingungen mechanischer Antriebssysteme spatially resolved spectroscopy and present preliminary BBXRT results on several clusters. The BBXRT results are in good agreement with simple cooling flow theory, in 3 cases confirm the existence of cold material in the cluster, find only shallow abundance gradients and constrain the mass profile in the central regions of the cluster.作者: engrave 時(shí)間: 2025-4-1 05:14 作者: Intervention 時(shí)間: 2025-4-1 06:45
Einfache lineare Schwingungssysteme,lusters, up to ~ 100 ~ 150 Mpc in scale, is suggested. The supercluster network surrounds low-density regions of similar scales, suggesting a “cellular” structure of the universe. (H. = 100 km /s/ Mpc is used throughout.)作者: ANTE 時(shí)間: 2025-4-1 13:34
Book 1992 of wavelengths, from radio to X-ray which hasprovoked much theoretical debate and advanced our understanding of therecent evolution of the large-scale structure of the Universe. Thecurrent status of the subject is reviewed in this volume by activeresearchers who lectured at a NATO Advanced Study In作者: 從容 時(shí)間: 2025-4-1 18:24 作者: Bumptious 時(shí)間: 2025-4-1 19:06 作者: tackle 時(shí)間: 2025-4-2 02:04
