Quasars in the 4D Eigenvector 1 Context: A stroll down memory lane
Jack W. Sulentic, Paola Marziani

TL;DR
This paper reviews 15 years of progress in understanding quasars through 4D Eigenvector 1 analysis, highlighting advances in phenomenology, unification models, and remaining challenges.
Contribution
It synthesizes developments in quasar spectroscopy using eigenvector techniques, proposing a unifying framework based on the 4D Eigenvector 1 context.
Findings
Eigenvector techniques reveal quasar main sequence driven by Eddington ratio and orientation.
Differences between population A and B quasars suggest a unified physical model.
Progress made over 15 years enhances understanding of quasar phenomenology.
Abstract
Recently some pessimism has been expressed about our lack of progress in understanding quasars over the 50+ year since their discovery. It is worthwhile to look back at some of the progress that has been made - but still lies under the radar - perhaps because few people are working on optical/UV spectroscopy in this field. Great advances in understanding quasar phenomenology have emerged using eigenvector techniques. The 4D eigenvector 1 context provides a surrogate H-R Diagram for quasars with a source main sequence driven by Eddington ratio convolved with line-of-sight orientation. Appreciating the striking differences between quasars at opposite ends of the main sequence (so-called population A and B sources) opens the door towards a unified model of quasar physics, geometry and kinematics. We present a review of some of the progress that has been made over the past 15 years, and…
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