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Titlebook: Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies; Christopher Mark Harrison Book 2016 The

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发表于 2025-3-21 16:24:33 | 显示全部楼层 |阅读模式
书目名称Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies
编辑Christopher Mark Harrison
视频video
概述Nominated as an outstanding Ph.D. thesis by the Durham University, UK.Demonstrates that the currently accepted models of galaxy formation are correct in parts but have parts that are not reproduced by
丛书名称Springer Theses
图书封面Titlebook: Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies;  Christopher Mark Harrison Book 2016 The
描述This prize-winning Ph.D. thesis by Chris Harrison adopts a multi-faceted approach to address the lack of decisive observational evidence, utilising large observational data sets from several world-leading telescopes. Developing several novel observational techniques, Harrison demonstrated that energetic winds driven by Active Galactic Nuclei (AGN) are found in a large number of galaxies, with properties in agreement with model predictions. One of the key unsolved problems in astrophysics is understanding the influence of AGN, the sites of growing supermassive black holes, on the evolution of galaxies. Leading theoretical models predict that AGN drive energetic winds into galaxies, regulating the formation of stars. However, until now, we have lacked the decisive observational evidence to confirm or refute these key predictions. Careful selection of targets allowed Harrison, to reliably place these detailed observations into the context of the overall galaxy population. However, in disagreement with the model predictions, Harrison showed that AGN have little global effect on star formation in galaxies. Theoretical models are now left with the challenge of explaining these results.
出版日期Book 2016
关键词Galaxy evolution; AGN Feedback Observations; Active Galactic Nuclei; IFU Observations of AGN; IFU Observ
版次1
doihttps://doi.org/10.1007/978-3-319-28454-5
isbn_softcover978-3-319-80357-9
isbn_ebook978-3-319-28454-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
issn_series 2190-5053
copyrightThe Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerl
The information of publication is updating

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发表于 2025-3-21 22:00:11 | 显示全部楼层
Christopher Mark Harrisoneignet sind..Der Autor..Lars Franke ist in der Entwicklung von maßgeschneiderten Enzymen für die Peptidsynthese und Proteinmodifizierung am Charles-Tannford-Proteinzentrum in Halle tätig..978-3-658-30436-2978-3-658-30437-9
发表于 2025-3-22 01:25:39 | 显示全部楼层
2190-5053 r, in disagreement with the model predictions, Harrison showed that AGN have little global effect on star formation in galaxies. Theoretical models are now left with the challenge of explaining these results.978-3-319-80357-9978-3-319-28454-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
发表于 2025-3-22 07:26:39 | 显示全部楼层
Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies
发表于 2025-3-22 09:29:07 | 显示全部楼层
Energetic Galaxy-Wide Outflows in High-, ULIRGs Hosting AGN Activity,emely broad [O .] emission-line profiles (FWHM . 700–1400 km s.) across . 4–15 kpc (i.e., across the extent of the host galaxies). The four less powerful AGN display weaker evidence for spatially extended outflows; however, this may be due, in-part, to the lower quality data for these objects. We es
发表于 2025-3-22 16:44:48 | 显示全部楼层
Kiloparsec Scale Outflows Are Prevalent in Luminous AGN: Outflows and Feedback in the Context of thd spatial extents of .(6–16) kpc in all targets. We show that our targets are representative of ., type 2 quasars and that ionised outflows are not only common but also in .70 % (3. confidence) of cases, they are extended over kiloparsec scales. Both star formation and AGN activity appear to be ener
发表于 2025-3-22 20:29:53 | 显示全部楼层
,Storm in a “Teacup”: A Radio-Quiet Quasar with ,10 kpc Radio-Emitting Bubbles and Extreme Gas Kinemof mechanical energy input from this AGN, despite it being formally “radio quiet”. Our study highlights that even when a quasar is formally “radio-quiet” the radio emission can be extremely effective for observing the effects of AGN feedback.
发表于 2025-3-22 21:57:46 | 显示全部楼层
No Submillimetre Signature of Star Formation Suppression Among X-Ray Luminous AGN,ude improvement in the number of sources at . in the same redshift range. By using these data to measure the star formation rates as a function of AGN power, we find no evidence for suppressed star formation in the most luminous AGN. The mean SFRs of the AGN are constant over the broad X-ray luminos
发表于 2025-3-23 04:22:26 | 显示全部楼层
Book 2016lace these detailed observations into the context of the overall galaxy population. However, in disagreement with the model predictions, Harrison showed that AGN have little global effect on star formation in galaxies. Theoretical models are now left with the challenge of explaining these results.
发表于 2025-3-23 05:37:57 | 显示全部楼层
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