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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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Citations
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Near-Infrared Spectroscopy of Seyfert Galaxies. Nuclear Activity and Stellar Population

TL;DR: In this article, the authors used the long-slit spectra of five Seyfert galaxies with jet-gas interaction to study the excitation and ionization mechanisms that are dominating the narrow-line region emission of these objects, that is affected by the radio-jet interaction.
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High-Ionization Nuclear Emission-Line Region of Seyfert Galaxies

TL;DR: In this paper, the authors applied the high-ionization nuclear emission-line region (HINER) test on 124 Seyfert nuclei to investigate the viewing angle toward the dusty torus.
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An XMM-Newton Observation of the Luminous Seyfert 1 Galaxy Markarian 509

TL;DR: In this article, the spectral analysis of an early XMM-Newton observation of the luminous Seyfert 1 galaxy Mrk 509 was presented, and it was shown that the hard (2-10 keV) continuum slope, including reflection, is somewhat flatter (? = 1.75) than that of a typical broad-line SEYFERT 1 galaxy.
Journal ArticleDOI

The Multitude of Unresolved Continuum Sources at 1.6 Microns in Hubble Space Telescope Images of Seyfert Galaxies

TL;DR: In this article, the authors examined 112 Seyfert galaxies observed by the Hubble Space Telescope at 1.6 km and found that about 50% of the galaxies have unresolved continuum sources.
Journal ArticleDOI

2WHSP: A multi-frequency selected catalogue of high energy and very high energy γ-ray blazars and blazar candidates

TL;DR: In this article, the authors presented the 2WHSP sample, the largest and most complete list of high synchrotron peaked blazars available to date, which is an expansion of the 1WHSP catalogue of γ-ray source candidates off the Galactic plane.
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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