標題: Titlebook: Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies; Christopher Mark Harrison Book 2016 The [打印本頁] 作者: cherub 時間: 2025-3-21 16:24
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書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies被引頻次學科排名
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書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies讀者反饋
書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies讀者反饋學科排名
作者: Suppository 時間: 2025-3-21 22:00
Christopher Mark Harrisoneignet sind..Der Autor..Lars Franke ist in der Entwicklung von ma?geschneiderten Enzymen für die Peptidsynthese und Proteinmodifizierung am Charles-Tannford-Proteinzentrum in Halle t?tig..978-3-658-30436-2978-3-658-30437-9作者: 完成才能戰(zhàn)勝 時間: 2025-3-22 01:25
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 作者: Androgen 時間: 2025-3-22 07:26
Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies作者: SMART 時間: 2025-3-22 09:29
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作者: ALT 時間: 2025-3-22 16:44
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作者: SHOCK 時間: 2025-3-22 20:29
,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.作者: HAWK 時間: 2025-3-22 21:57
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作者: CRUMB 時間: 2025-3-23 04:22
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.作者: LAP 時間: 2025-3-23 05:37 作者: inclusive 時間: 2025-3-23 13:19 作者: Bouquet 時間: 2025-3-23 16:30 作者: 牢騷 時間: 2025-3-23 19:19 作者: 潰爛 時間: 2025-3-23 23:03 作者: 出處 時間: 2025-3-24 04:12
,Storm in a “Teacup”: A Radio-Quiet Quasar with ,10?kpc Radio-Emitting Bubbles and Extreme Gas Kinemuasars? In this pilot study, we present VLA radio and VIMOS IFU observations of the radio-quiet, type?2 quasar that has been nicknamed the “Teacup AGN” due to it emission-line region morphology. In the central .1?kpc we observe a high-velocity ionised outflow that is co-spatial with a radio structur作者: 頌揚本人 時間: 2025-3-24 06:54
No Submillimetre Signature of Star Formation Suppression Among X-Ray Luminous AGN,rates compared to the galaxy population as a whole? Many theoretical models require powerful active galactic nuclei (AGN) to suppress star formation in distant galaxies in order to reproduce the observed properties of today’s massive galaxies. The observational work that has been investigating the s作者: Chipmunk 時間: 2025-3-24 12:47
Conclusions,ter summarises the main results from the work presented in this thesis and the main outstanding issues that are still to be addressed. On-going and future projects, to address these outstanding issues are described, along with some of the preliminary results, in the following chapter.作者: fleeting 時間: 2025-3-24 18:33
Ongoing and Future Work,. However, as outlined in the previous chapter, there are outstanding questions that still need to be addressed. As a result of the work presented in this thesis, a number of follow-up observational projects are now underway to answer some of these questions. In this chapter we consider four of the 作者: Dappled 時間: 2025-3-24 19:43 作者: 虛弱的神經(jīng) 時間: 2025-3-25 01:56 作者: 剝削 時間: 2025-3-25 06:53 作者: acheon 時間: 2025-3-25 11:14 作者: obstruct 時間: 2025-3-25 13:34 作者: 楓樹 時間: 2025-3-25 18:12 作者: SIT 時間: 2025-3-25 23:01 作者: 失望未來 時間: 2025-3-26 02:34 作者: Solace 時間: 2025-3-26 06:33 作者: escalate 時間: 2025-3-26 12:32
Ongoing and Future Work,outflows in AGN?; (2) what are the multi gas-phase properties of galaxy-wide outflows?; (3) what is the prevalence of ionised outflows in galaxies across cosmic time?; and (4) what impact do outflows have on galaxy evolution? We finish this chapter with some final remarks on the status of the research that has been covered in this thesis.作者: BOAST 時間: 2025-3-26 16:20
Book 2016rge 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作者: 無可非議 時間: 2025-3-26 18:58 作者: 好色 時間: 2025-3-26 21:07 作者: 鐵砧 時間: 2025-3-27 03:55 作者: Munificent 時間: 2025-3-27 07:51
https://doi.org/10.1007/978-3-658-37793-9fers a taste of 3D before Flash ever hit the market. VRML was a great idea, but it was ahead of its time and, sadly, didn’t go very far. In any case, it was more of a programmer’s pursuit than something a designer would want to grapple with.作者: HAUNT 時間: 2025-3-27 09:41
Detection of Disruption of Sarcolemmal Membrane by Indium-111 Labeled Antimyosin Antibody Scanve heart failure, chest pain, fatigue, dizzy spells, and even syncope or cardiac arrest. In our daily practice these symptoms are not specific, and we may misdiagnose them as coronary disease, idiopathic dilated cardiomyopathy, or other noncardiac disorders. This can be exemplified by the following case.作者: yohimbine 時間: 2025-3-27 13:44 作者: SLING 時間: 2025-3-27 18:17
Resilience in Supply Chain Managementure. The process entails associating the image with a class of sources with common characteristics (device model) or matching the image to an individual source device, for example a specific camera. Third, attesting to the integrity of image data. This involves image forgery detection to determine w作者: Ingratiate 時間: 2025-3-28 00:11 作者: AFFIX 時間: 2025-3-28 02:47 作者: aviator 時間: 2025-3-28 09:44
Marcus Herntreiibed to the increase in the entropy that occurs during the polymerization of these monomers. This increase in entropy is based on the increase in the degrees of freedom of rotation gained when rings are transformed into open chains.作者: 外露 時間: 2025-3-28 11:15 作者: Increment 時間: 2025-3-28 16:08 作者: 松緊帶 時間: 2025-3-28 19:35
