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010   $a3-319-28454-1
024 7 $a10.1007/978-3-319-28454-5
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035   $a(PQKBTitleCode)TC0001607037
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035   $a(DE-He213)978-3-319-28454-5
035   $a(MiAaPQ)EBC4354094
035   $a(PPN)191706507
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100   $a20160120d2016      u|         0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aObservational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies /$fby Christopher Mark Harrison
205   $a1st ed. 2016.
210  1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2016.
215   $a1 online resource (208 p.)
225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
300   $aDescription based upon print version of record.
311   $a3-319-28453-3 
320   $aIncludes bibliographical references at the end of each chapters and index.
327   $aIntroduction -- Integral field spectroscopy and spectral energy distributions -- Energetic galaxy-wide outflows in high-z ULIRGs hosting AGN activity -- Kiloparsec scale outflows are prevalent in luminous AGN: outflows and feedback in the context of the overall AGN population -- Storm in a ?Teacup?: a radio-quiet quasar with ?10 kpc radio-emitting bubbles and extreme gas kinematics -- No submillimetre signature of star formation suppression among X-ray luminous AGN -- Conclusions -- Ongoing and future work.
330   $aThis prize-winning Ph.D. thesis by Chris Harrison adopts a multi-faceted approach to address the lack of decisive observational evidence, utilising large observational data sets from several world-leading telescopes. Developing several novel observational techniques, Harrison demonstrated that energetic winds driven by Active Galactic Nuclei (AGN) are found in a large number of galaxies, with properties in agreement with model predictions. One of the key unsolved problems in astrophysics is understanding the influence of AGN, the sites of growing supermassive black holes, on the evolution of galaxies. Leading theoretical models predict that AGN drive energetic winds into galaxies, regulating the formation of stars. However, until now, we have lacked the decisive observational evidence to confirm or refute these key predictions. Careful selection of targets allowed Harrison, to reliably place these detailed observations into the context of the overall galaxy population. However, in disagreement with the model predictions, Harrison showed that AGN have little global effect on star formation in galaxies. Theoretical models are now left with the challenge of explaining these results.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aAstrophysics
606   $aObservations, Astronomical
606   $aAstronomy?Observations
606   $aCosmology
606   $aAstrophysics and Astroparticles$3https://scigraph.springernature.com/ontologies/product-market-codes/P22022
606   $aAstronomy, Observations and Techniques$3https://scigraph.springernature.com/ontologies/product-market-codes/P22014
606   $aCosmology$3https://scigraph.springernature.com/ontologies/product-market-codes/P22049
615  0$aAstrophysics.
615  0$aObservations, Astronomical.
615  0$aAstronomy?Observations.
615  0$aCosmology.
615 14$aAstrophysics and Astroparticles.
615 24$aAstronomy, Observations and Techniques.
615 24$aCosmology.
676   $a523.112
700   $aHarrison$b Christopher Mark$4aut$4http://id.loc.gov/vocabulary/relators/aut$0288817
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910254618203321
996   $aObservational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies$91811502
997   $aUNINA