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Journal ArticleDOI

Unified models for active galactic nuclei and quasars

Robert Antonucci
- 01 Jan 1993 - 
- Vol. 31, Iss: 1, pp 473-521
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TLDR
The straw person model (SPM) as mentioned in this paper has been proposed to explain the orientation effects of active galactic nuclei (AGN) and quasars in the line of sight (LOS) images.
Abstract
Because the critical central regions of Active Galactic Nuclei (AGN) and quasars are strongly nonspherical but spatially unresolved, orientation effects have been the source of much confusion. In fact, it now appears that much of the variety in AGN types is just the result of varying orientation relative to the line of sight. We can define an extreme hypothesis,, the straw person model (SPM), in which there are two basic types of AGN: the radio quiets and the radio louds. For each type there is a range in intrinsic luminosity, and the luminosity controls some properties such as the Fanaroff and Riley classes. However, at a given intrinsic luminosity, all other properties such as spectroscopic classification and VLBI component speeds are ascribed to orientation. This model is only a caricature of the unification idea, and is already ruled out on many grounds, but it will be useful for organizing the discussion. I’ll describe what I consider to be convincing evidence that orientation effects are important and widespread. The true situation may be in some sense half way between the SPM and the hypothesis that orientation doesn’t affect classification at aIl. To us optimists, the orienration cup is half full rather than half empty. Although it is too soon to say for sure, the hypothesis that most objects’ classifications would be different if seen from other directions is a tenable one today.

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Journal ArticleDOI

The nature of the molecular gas system in the core of NGC 1275

TL;DR: In this paper, the authors present near-infrared integral field spectroscopy of the central kiloparsec of NGC 1275 at the heart of the Perseus cluster of galaxies, obtained with the Integral Field Unit (IFU) of the United Kingdom Infrared Telescope (UKIRT) Imaging Spectrometer (UIST).
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The bolometric quasar luminosity function at z = 0–7

TL;DR: In this article, the authors provide updated constraints on the bolometric quasar luminosity function (QLF) from 0 to 7, based on an observational compilation that includes observations in the rest-frame, IR, B band, UV, soft and hard X-ray in past decades.
Journal ArticleDOI

Radio Loud and Radio Quiet Active Galactic Nuclei

TL;DR: In this article, the authors show that the radio luminosity at 5 GHz and the line luminosity in [OIII] 5007 have been correlated in a similar way for both radio-loud and radio-quiet AGNs, and demonstrate that the observed correlation can be explained in terms of a model in which jets are accelerated and collimated by a vertical magnetic field.
References
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Journal ArticleDOI

Phd by thesis

TL;DR: In this paper, a sedimentological core and petrographic characterisation of samples from eleven boreholes from the Lower Carboniferous of Bowland Basin (Northwest England) is presented.
Journal Article

Superluminal Radio Sources

J. A. Zensus, +1 more
- 01 Aug 1982 - 
TL;DR: There are now at least 23 radio sources in which apparent superluminal motion has been found as mentioned in this paper, and the effect is not limited to the classic examples like 3C 345, but is found in objects with a wide range of characteristic properties.
Journal ArticleDOI

Superluminal radio sources

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