scispace - formally typeset
Journal ArticleDOI

Unified models for active galactic nuclei and quasars

Robert Antonucci
- 01 Jan 1993 - 
- Vol. 31, Iss: 1, pp 473-521
Reads0
Chats0
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.

read more

Citations
More filters
Journal ArticleDOI

AGN Type-casting: Mrk 590 No Longer Fits the Role

TL;DR: In this paper, the authors present multi-wavelength observations that trace more than 40 years in the life of the active galactic nucleus (AGN) in Mrk 590, traditionally known as a classic Seyfert 1 galaxy.
Journal ArticleDOI

Radio-loud and radio-quiet active galactic nuclei

TL;DR: In this paper, the authors have generated a sample of 409 active galactic nuclei (AGNs) for which both the radio luminosity at 5 GHz and the line luminosity in [O III]?5007 have been measured, showing that these two quantities are correlated in a similar way for both radio-loud and radio-quiet AGNs.
Journal ArticleDOI

The role of molecular gas in obscuring seyfert active galactic nuclei

TL;DR: In this paper, a sample of local active galactic nuclei (AGNs) was studied at a spatial resolution on the order of 10 pc, and it was shown that the interstellar medium traced by the molecular hydrogen = 1-0 S(1) line at 2.1?m forms a geometrically thick, clumpy disk.
Journal ArticleDOI

A combined optical and X-ray study of unobscured type 1 active galactic nuclei – I. Optical spectra and spectral energy distribution modelling

TL;DR: In this paper, the authors used the spectral properties of active galactic nuclei (AGNs) to derive the intrinsic optical continuum and derive the properties of the underlying accretion disc.
References
More filters
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

Related Papers (5)