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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

The Quasar Main Sequence Explained by the Combination of Eddington Ratio, Metallicity, and Orientation

TL;DR: In this paper, the effect of orientation of the accretion disk plane and the geometry of the broad-line region (BLR) on the distribution of quasars in the optical plane of the quasar main sequence was investigated.
Journal ArticleDOI

XMM-Newton broad-band observations of NGC 7582: N{H} variations and fading out of the active nucleus

TL;DR: In this paper, the authors present results from two XMM-Newton observations of the bright classical Seyfert 2 galaxy NGC 7582 taken four years apart (2001 May and 2005 April).
Journal ArticleDOI

[O III]$\lambda 5007$ and X-ray Properties of a Complete Sample of Hard X-ray Selected AGNs in the Local Universe

TL;DR: In this article, the authors studied the correlation between the [O III]$\lambda 5007$ and X-ray luminosities of local Active Galactic Nuclei (AGNs), using a complete, hard Xray ($>10$ keV) selected sample in the Swift/BAT 9-month catalog.
Dissertation

Measuring the Hubble constant from reverberating accretion discs in active galaxies

TL;DR: In this article, wavelength-dependent time delays between continuum flux variations of active galactic nuclei (AGNs) can be used to test the standard black hole-accretion disc paradigm, by measuring the temperature structure TORU of the gaseous material surrounding the purported black hole.
Journal ArticleDOI

The Far-Infrared Spectral Energy Distributions of X-ray-selected Active Galaxies

TL;DR: In this paper, the authors compare the far-IR spectral energy distributions (SEDs) of a hard X-ray AGN sample with various radio and optically selected AGN samples.
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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