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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書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies影響因子(影響力)




書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies影響因子(影響力)學(xué)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網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies被引頻次




書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies被引頻次學(xué)科排名




書目名稱Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies年度引用




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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(xué)科排名

Suppository

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

完成才能戰(zhàn)勝

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

Androgen

Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies

SMART

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

ALT

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

SHOCK

,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.

HAWK

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

CRUMB

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.

LAP