找回密碼
 To register

QQ登錄

只需一步,快速開始

掃一掃,訪問微社區(qū)

打印 上一主題 下一主題

Titlebook: Disc Winds Matter; Modelling Accretion James Matthews Book 2017 Springer International Publishing AG 2017 Astrophysical Outflows.Accretion

[復制鏈接]
查看: 32653|回復: 41
樓主
發(fā)表于 2025-3-21 17:59:46 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Disc Winds Matter
副標題Modelling Accretion
編輯James Matthews
視頻videohttp://file.papertrans.cn/281/280897/280897.mp4
概述Nominated as an outstanding PhD thesis by the University of Southampton, Southampton, UK.Includes a broad introduction to accretion and outflow in astrophysical systems.Features a detailed description
叢書名稱Springer Theses
圖書封面Titlebook: Disc Winds Matter; Modelling Accretion  James Matthews Book 2017 Springer International Publishing AG 2017 Astrophysical Outflows.Accretion
描述.This thesis describes the application of a Monte Carlo radiative transfer code to accretion disc winds in two types of systems spanning 9 orders of magnitude in mass and size. In both cases, the results provide important new insights.?On small scales, the presence of disc winds in accreting white dwarf binary systems has long been inferred from the presence of ultraviolet absorption lines.?Here, the thesis shows that the same winds can also produce optical emission lines and a recombination continuum.?On large scales, the thesis constructs a simple model of disc winds in quasars that is capable of explaining both the observed absorption and emission signatures – a crucial advance that supports a disc-wind based unification scenario for quasars.?Lastly, the thesis also includes a theoretical investigation into the equivalent width distribution of the emission lines in quasars, which reveals a major challenge to all unification scenarios..
出版日期Book 2017
關鍵詞Astrophysical Outflows; Accretion Disc Winds; Quasars and Active Galactic Nuclei; Radiative Transfer in
版次1
doihttps://doi.org/10.1007/978-3-319-59183-4
isbn_softcover978-3-319-86563-8
isbn_ebook978-3-319-59183-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightSpringer International Publishing AG 2017
The information of publication is updating

書目名稱Disc Winds Matter影響因子(影響力)




書目名稱Disc Winds Matter影響因子(影響力)學科排名




書目名稱Disc Winds Matter網(wǎng)絡公開度




書目名稱Disc Winds Matter網(wǎng)絡公開度學科排名




書目名稱Disc Winds Matter被引頻次




書目名稱Disc Winds Matter被引頻次學科排名




書目名稱Disc Winds Matter年度引用




書目名稱Disc Winds Matter年度引用學科排名




書目名稱Disc Winds Matter讀者反饋




書目名稱Disc Winds Matter讀者反饋學科排名




單選投票, 共有 0 人參與投票
 

0票 0%

Perfect with Aesthetics

 

0票 0%

Better Implies Difficulty

 

0票 0%

Good and Satisfactory

 

0票 0%

Adverse Performance

 

0票 0%

Disdainful Garbage

您所在的用戶組沒有投票權限
沙發(fā)
發(fā)表于 2025-3-21 20:53:22 | 只看該作者
2190-5053 that supports a disc-wind based unification scenario for quasars.?Lastly, the thesis also includes a theoretical investigation into the equivalent width distribution of the emission lines in quasars, which reveals a major challenge to all unification scenarios..978-3-319-86563-8978-3-319-59183-4Series ISSN 2190-5053 Series E-ISSN 2190-5061
板凳
發(fā)表于 2025-3-22 00:38:46 | 只看該作者
James MatthewsNominated as an outstanding PhD thesis by the University of Southampton, Southampton, UK.Includes a broad introduction to accretion and outflow in astrophysical systems.Features a detailed description
地板
發(fā)表于 2025-3-22 06:49:12 | 只看該作者
5#
發(fā)表于 2025-3-22 09:45:18 | 只看該作者
6#
發(fā)表于 2025-3-22 13:12:39 | 只看該作者
7#
發(fā)表于 2025-3-22 17:05:01 | 只看該作者
Aphabetical Index of substances,Observational evidence for mass-loaded outflows or winds is widespread across the entire astrophysical mass range and most of the electromagnetic spectrum.
8#
發(fā)表于 2025-3-22 21:24:23 | 只看該作者
9#
發(fā)表于 2025-3-23 01:41:06 | 只看該作者
Space groups (194) P63/mmc - (190) P-62cHere, I present Monte Carlo radiative transfer simulations designed to assess the likely impact of accretion disc winds on the optical spectra of high-state CVs.
10#
發(fā)表于 2025-3-23 07:22:16 | 只看該作者
Space groups (189) P-62m – (174) P-6In Chaps.?. and ., I reviewed the observational evidence for accretion disc winds in quasars and luminous AGN, and showed how they may be responsible for more than just the broad absorption lines and P-Cygni profiles seen in quasar spectra.
 關于派博傳思  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 論文服務流程 影響因子官網(wǎng) 吾愛論文網(wǎng) 大講堂 北京大學 Oxford Uni. Harvard Uni.
發(fā)展歷史沿革 期刊點評 投稿經(jīng)驗總結(jié) SCIENCEGARD IMPACTFACTOR 派博系數(shù) 清華大學 Yale Uni. Stanford Uni.
QQ|Archiver|手機版|小黑屋| 派博傳思國際 ( 京公網(wǎng)安備110108008328) GMT+8, 2025-10-14 18:11
Copyright © 2001-2015 派博傳思   京公網(wǎng)安備110108008328 版權所有 All rights reserved
快速回復 返回頂部 返回列表
西平县| 栾城县| 九龙城区| 施秉县| 龙里县| 双辽市| 敦化市| 汉沽区| 大冶市| 东安县| 邛崃市| 南川市| 金阳县| 桃源县| 弋阳县| 灯塔市| 彩票| 类乌齐县| 盐津县| 仁化县| 左权县| 太白县| 兰考县| 鲜城| 景德镇市| 广汉市| 宝丰县| 苍梧县| 时尚| 吴桥县| 新建县| 渝北区| 镇远县| 元谋县| 资讯 | 深水埗区| 海伦市| 平湖市| 勃利县| 武平县| 方城县|