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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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Journal ArticleDOI

What broad emission lines tell us about how active galactic nuclei work

TL;DR: In this paper, the authors review progress made in understanding the nature of the broad-line region (BLR) of active galactic nuclei and the role BLRs play in the AGN phenomenon.
Journal ArticleDOI

The Star-forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC 3227*

TL;DR: In this article, the authors presented the morphologies and kinematics of emission lines and absorption features and gave the first derivation of a black hole mass in a Seyfert 1 nucleus from stellar dynamics.
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Testing thermal reprocessing in active galactic nuclei accretion discs

TL;DR: In this paper, the authors fit the observed time-delays and optical spectral energy distribution using a disc reprocessing model, which delivers estimates for the nuclear reddening, the product of black hole mass and accretion rate, and the distance to each object.
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Resolving the obscuring torus in NGC 1068 with the power of infrared interferometry: revealing the inner funnel of dust

TL;DR: In this paper, the authors used MIDI data obtained with the MIDI (MID infrared Interferometric instrument) for the Seyfert II galaxy NGC 1068 to obtain an image of the source using maximum entropy image reconstruction.

Report on the ESO Workshop ''Active Galactic Nuclei: what's in a name?''

P. Padovani
TL;DR: In this paper, an overview of AGN multi-wavelength properties with the aim of painting their "big picture" through observations in each electromagnetic band from radio to gamma-rays as well as AGN variability.
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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