標(biāo)題: Titlebook: Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena; Richard Lieu,Jonathan Mittaz Conference proceedings 2004 Springer Sci [打印本頁] 作者: 審美家 時(shí)間: 2025-3-21 18:11
書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena影響因子(影響力)
書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena影響因子(影響力)學(xué)科排名
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書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena被引頻次
書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena被引頻次學(xué)科排名
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書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena讀者反饋
書目名稱Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena讀者反饋學(xué)科排名
作者: 拉開這車床 時(shí)間: 2025-3-21 21:15
scipline would at least require that we have stocks of useful off-the-shelf programs and collections of standard theorems that can be applied repeatedly. We have neither..Mathematical systems are often distinguished by a set of operations that (a) map a set of entities into itself, (b) have simply u作者: 廚房里面 時(shí)間: 2025-3-22 04:11 作者: Perineum 時(shí)間: 2025-3-22 06:52 作者: Harness 時(shí)間: 2025-3-22 11:58
M. Bonamente,M. K. Joy,R. Lieuscipline would at least require that we have stocks of useful off-the-shelf programs and collections of standard theorems that can be applied repeatedly. We have neither..Mathematical systems are often distinguished by a set of operations that (a) map a set of entities into itself, (b) have simply u作者: Favorable 時(shí)間: 2025-3-22 13:35
J. Nevalainen,R. Lieu,M. Bonamente,D. Lumbareas such as error-correcting codes, cryptography, the safety and security critical fields, the banking and insurance fields, as well as traditional engineering applications.?.Topics and features:..Addressescore mathematics for critical thinking and problem solving..Discussespropositional and predi作者: Colonoscopy 時(shí)間: 2025-3-22 17:19 作者: Detoxification 時(shí)間: 2025-3-23 00:33 作者: OGLE 時(shí)間: 2025-3-23 03:00 作者: frozen-shoulder 時(shí)間: 2025-3-23 07:38
itical performance is paramount, such as in aircraft, missiles, nuclear reactors and weapons, submarines, and many other types of systems where “failure” can result in overwhelming loss of life and property. The book is divided into four parts: Fundamentals, Electronics, Software, and Dangerous Good作者: 友好關(guān)系 時(shí)間: 2025-3-23 09:54
T. Fang,C. Canizares,K. Sembach,H. Marshall,J. Lee,D. Davisftware modules usually varies with time according to a Rayleigh distribution (Peterson and Arellano in Reliability Review, 22, .). However, the normalized failure rates . in the “tails” (large values of time) are higher than those predicted by the Rayleigh model. And, the normalized failure rate his作者: Anthrp 時(shí)間: 2025-3-23 14:32 作者: entice 時(shí)間: 2025-3-23 18:53 作者: BROOK 時(shí)間: 2025-3-24 00:28 作者: 尋找 時(shí)間: 2025-3-24 04:30
Conference proceedings 2004 launch of new missions such as XMM-Newton and FUSE, we are beginning to answer some of the complex issues regarding the phenomenon. This conference proceedings is an attempt to bring together the latest research results and covers both observational and theoretical work on the CSE and related topic作者: 平 時(shí)間: 2025-3-24 09:27
The Extreme Ultraviolet Excess Emission in Five Clusters of Galaxies Revisitedfidence level and an EUV excess over a thermal bremsstrahlung tail is detected in all five clusters (Abell 1795, Abell 2199, Abell 4059, Coma and Virgo) up to large radii. Our results tend to suggest that the EUV excess is probably non thermal in origin.作者: neutralize 時(shí)間: 2025-3-24 12:25 作者: 愛哭 時(shí)間: 2025-3-24 18:38
A Massive Halo of Warm Baryons in the Coma Clustern from warm gas at ~ 10. K. The mass of the warm gas is on par with that of the hot X-ray emitting plasma, and significantly more massive if the warm gas resides in low-density filamentary structures.作者: 吼叫 時(shí)間: 2025-3-24 21:22
XMM-Newton Discovery of an X-Ray Filament in ComaOur measurements provide a direct estimate of the O, Ne and Fe abundance of the WHIM. Differences with the reported Ne/O ratio for some OVI absorbers hints to different origin of the OVI absorbers and the Coma filament.作者: 不安 時(shí)間: 2025-3-25 02:31
The Ism from the Soft X-ray Background Perspectivet indicates that O VI emission from the Local Hot Bubble is insignificant, if it exists at all, a result which is also inconsistent with current thermal emission models. A (very) short review of the Galactic SXRB and ISM is presented.作者: Acetaminophen 時(shí)間: 2025-3-25 05:01 作者: JECT 時(shí)間: 2025-3-25 08:45
Soft (1 KEV) X-Ray Emission in Galaxy Clusterswe find evidence of a soft excess that can be modeled either as thermal emission or as non-thermal emission. For IC 1262, the thermal interpretation is nonphysical and the non-thermal model has further support from a radio halo that we propose exists in the cluster center. For Abell 754, we modeled 作者: MELON 時(shí)間: 2025-3-25 14:59 作者: Obedient 時(shí)間: 2025-3-25 16:23 作者: SPASM 時(shí)間: 2025-3-25 20:01
XMM-Newton Discovery of O VII Emission from Warm Gas in Clusters of Galaxiesbuted to the Warm-Hot Intergalactic Medium. The original sample of clusters studied for this purpose has been extended and two more clusters with a soft X-ray excess have been found. We discuss the physical properties of the warm gas, in particular the density, spatial extent, abundances and tempera作者: Anthrp 時(shí)間: 2025-3-26 02:38 作者: 葡萄糖 時(shí)間: 2025-3-26 06:50 作者: defeatist 時(shí)間: 2025-3-26 10:59 作者: Euphonious 時(shí)間: 2025-3-26 15:12
The Fuse Survey of O VI in the Galactic Haloc objects and two distant halo stars are analyzed to obtain measures of O VI absorption along paths through the Milky Way thick disk/halo. Strong O VI absorption over the velocity range from —100 to 100 km s. reveals a widespread but highly irregular distribution of O VI, implying the existence of s作者: 吸引力 時(shí)間: 2025-3-26 17:37 作者: 殘忍 時(shí)間: 2025-3-26 22:24 作者: diabetes 時(shí)間: 2025-3-27 04:06
The Ism from the Soft X-ray Background Perspective been seen as it has been about detections. High resolution spectra of the local SXRB have been observed, but are inconsistent with current thermal emission models. An excess over the extrapolation of the high-energy (most clearly visible at . 1.5 keV) extragalactic power law down to ? keV has been 作者: 特別容易碎 時(shí)間: 2025-3-27 06:56 作者: Cupping 時(shí)間: 2025-3-27 09:36 作者: faculty 時(shí)間: 2025-3-27 15:49
Soft X-Ray Excess Emission in Three Clusters of Galaxies Observed with XMM-Newtona large fraction of the current epoch’s bayons located in a warm-hot intergalactic medium (WHIM). However, the derived densities are too high in the cluster cores, compared to WHIM simulations, and thus more theoretical work is needed to fully understand the origin of the observed soft X-ray excess.作者: aesthetician 時(shí)間: 2025-3-27 18:30
The Fuse Survey of High Velocity O VI in the Vicinity of the Milky Wayous galaxy formation scenarios. Additional spectroscopic data in the coming years will help to determine the ionization properties of the high velocity clouds and discriminate between the multiple types of high velocity O VI features found in this study.作者: 排斥 時(shí)間: 2025-3-27 23:32 作者: 紡織品 時(shí)間: 2025-3-28 03:50
The Cluster Abell 85 and its X-ray Filament Revisited by Chandra and XMM-NewtonV. This is significantly lower than the ambient cluster medium, but is significantly higher than anticipated for a gas in a weakly bound extended filament. It is not clear whether this is a filament of diffuse emission or a chain of several groups of galaxies.作者: Certainty 時(shí)間: 2025-3-28 06:51
0067-0057 the recent launch of new missions such as XMM-Newton and FUSE, we are beginning to answer some of the complex issues regarding the phenomenon. This conference proceedings is an attempt to bring together the latest research results and covers both observational and theoretical work on the CSE and rel作者: MUT 時(shí)間: 2025-3-28 10:48
Hard X-Ray Excesses in Clusters of Galaxies and Their Non-Thermal OriginThe first part of the paper reports all the results obtained by . observations concerning the search for non-thermal components in the spectra of clusters of galaxies, while the origin of the hard X-ray excesses detected in Coma, A2256 and, at lower confidence level, in A754 is discussed in the second part.作者: 后天習(xí)得 時(shí)間: 2025-3-28 17:22 作者: 星球的光亮度 時(shí)間: 2025-3-28 20:29
Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena978-1-4020-2564-8Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: Budget 時(shí)間: 2025-3-29 00:34 作者: 斷言 時(shí)間: 2025-3-29 03:51 作者: 進(jìn)取心 時(shí)間: 2025-3-29 08:20 作者: Antarctic 時(shí)間: 2025-3-29 15:26
Astrophysics and Space Science Libraryhttp://image.papertrans.cn/s/image/870618.jpg作者: WAG 時(shí)間: 2025-3-29 16:14
https://doi.org/10.1007/978-1-4020-2564-8Galaxy; Redshift; Universe; astronomy; stellar作者: GLUE 時(shí)間: 2025-3-29 20:15 作者: 含沙射影 時(shí)間: 2025-3-30 03:54
The Fuse Survey of O VI in the Galactic Halo including low and intermediate velocity H I, H. emission from the warm ionized gas at ~10. K, and hot X-ray emitting gas at ~40. K. The O VI has an average velocity dispersion, .=60 km s. and small standard deviation of 15 km s.. Thermal broadening alone cannot explain the large observed profile wi作者: eczema 時(shí)間: 2025-3-30 08:03 作者: 完成才會(huì)征服 時(shí)間: 2025-3-30 08:23
grams are the entities of just such a mathematical system: programs are built by program-forming operations having good algebraic properties. Hence they are the subject of a large number of general theorems, theorems that are applicable in practice. We give examples. Function level programs also hav作者: 指耕作 時(shí)間: 2025-3-30 13:27 作者: 切碎 時(shí)間: 2025-3-30 17:03
Florence Durret,Eric Slezak,Richard Lieu,Sergio Dos Santos,Massimiliano Bonamentegrams are the entities of just such a mathematical system: programs are built by program-forming operations having good algebraic properties. Hence they are the subject of a large number of general theorems, theorems that are applicable in practice. We give examples. Function level programs also hav作者: 瘋狂 時(shí)間: 2025-3-30 22:50
Mark Henriksengrams are the entities of just such a mathematical system: programs are built by program-forming operations having good algebraic properties. Hence they are the subject of a large number of general theorems, theorems that are applicable in practice. We give examples. Function level programs also hav作者: 蔓藤圖飾 時(shí)間: 2025-3-31 03:41 作者: 誘騙 時(shí)間: 2025-3-31 07:45
