This thesis is intended to give a general overview of one of the most forestanding research field of modern astrophysics: the quasar phenomenon. A description of the optical-UV spectroscopic properties and the spectral energy distribution is presented, followed by a discussion of the basic accretion mechanism and the different accretion modes. Then the thesis concentrates on the classification scheme of the FourDimensional Eigenvector 1 parameter space. The morphological properties of quasar hosts are also described. Finally, the thesis suggests a possible way to organize future morphological studies in the search for a connection between host morphology and the 4DE1 quasar sequence.

Quasars and their host galaxies I quasar e le loro galassie ospiti

Vanzani, Valeria
2016/2017

Abstract

This thesis is intended to give a general overview of one of the most forestanding research field of modern astrophysics: the quasar phenomenon. A description of the optical-UV spectroscopic properties and the spectral energy distribution is presented, followed by a discussion of the basic accretion mechanism and the different accretion modes. Then the thesis concentrates on the classification scheme of the FourDimensional Eigenvector 1 parameter space. The morphological properties of quasar hosts are also described. Finally, the thesis suggests a possible way to organize future morphological studies in the search for a connection between host morphology and the 4DE1 quasar sequence.
2016-10
40
Quasars, emission lines, host galaxy, active galactic nuclei, optical and UV spectroscopy, accretion disks
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12608/25016