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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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樓主: cherub
11#
發(fā)表于 2025-3-23 13:19:35 | 只看該作者
12#
發(fā)表于 2025-3-23 16:30:22 | 只看該作者
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發(fā)表于 2025-3-23 19:19:40 | 只看該作者
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發(fā)表于 2025-3-23 23:03:24 | 只看該作者
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發(fā)表于 2025-3-24 04:12:22 | 只看該作者
,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
16#
發(fā)表于 2025-3-24 06:54:41 | 只看該作者
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
17#
發(fā)表于 2025-3-24 12:47:20 | 只看該作者
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.
18#
發(fā)表于 2025-3-24 18:33:41 | 只看該作者
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
19#
發(fā)表于 2025-3-24 19:43:06 | 只看該作者
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發(fā)表于 2025-3-25 01:56:37 | 只看該作者
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