找回密碼
 To register

QQ登錄

只需一步,快速開(kāi)始

掃一掃,訪問(wèn)微社區(qū)

打印 上一主題 下一主題

Titlebook: Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena; Richard Lieu,Jonathan Mittaz Conference proceedings 2004 Springer Sci

[復(fù)制鏈接]
樓主: 審美家
11#
發(fā)表于 2025-3-23 09:54:00 | 只看該作者
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
12#
發(fā)表于 2025-3-23 14:32:50 | 只看該作者
13#
發(fā)表于 2025-3-23 18:53:27 | 只看該作者
14#
發(fā)表于 2025-3-24 00:28:02 | 只看該作者
15#
發(fā)表于 2025-3-24 04:30:36 | 只看該作者
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
16#
發(fā)表于 2025-3-24 09:27:33 | 只看該作者
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.
17#
發(fā)表于 2025-3-24 12:25:24 | 只看該作者
18#
發(fā)表于 2025-3-24 18:38:32 | 只看該作者
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.
19#
發(fā)表于 2025-3-24 21:22:07 | 只看該作者
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.
20#
發(fā)表于 2025-3-25 02:31:44 | 只看該作者
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.
 關(guān)于派博傳思  派博傳思旗下網(wǎng)站  友情鏈接
派博傳思介紹 公司地理位置 論文服務(wù)流程 影響因子官網(wǎng) 吾愛(ài)論文網(wǎng) 大講堂 北京大學(xué) Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點(diǎn)評(píng) 投稿經(jīng)驗(yàn)總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學(xué) Yale Uni. Stanford Uni.
QQ|Archiver|手機(jī)版|小黑屋| 派博傳思國(guó)際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-6 16:33
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權(quán)所有 All rights reserved
快速回復(fù) 返回頂部 返回列表
光山县| 阿拉善左旗| 顺昌县| 西宁市| 弥渡县| 韩城市| 上饶县| 红河县| 诸暨市| 新源县| 平原县| 云龙县| 镇坪县| 博客| 南康市| 营山县| 囊谦县| 广德县| 桂阳县| 新津县| 峨眉山市| 泾源县| 乐亭县| 盘锦市| 双城市| 沙河市| 哈巴河县| 万山特区| 中西区| 衡阳市| 宜章县| 锦州市| 松桃| 沙雅县| 卢氏县| 健康| 广宁县| 达拉特旗| 蛟河市| 虎林市| 湖南省|