1998arXiv (Cornell University)Open access

Jets in AGN -- New Results from HST and VLA

H. Falcke

Open full text 0 citations

Abstract

This paper summarizes some of our recent projects which try to illuminate the nature and importance of jets associated with active nuclei and compact objects. After a short introduction on jets in radio galaxies and radio loud quasars the paper focuses on jets in other source types, such as radio-quiet quasars, Seyfert and LINER galaxies, and stellar mass black holes. Radio observations of quasars, for example, have brought new evidence for the existence of relativistic jets in radio quiet quasars, while HST and VLA observations of Seyfert galaxies have now clearly established not only the presence of radio jets, but also the great importance these jets have for the morphology and the excitation of the emission line region in these AGN. Moreover, a recent VLA survey found a large fraction of low-luminosity AGN to host compact, flat-spectrum radio cores indicating the presence of radio jets there as well. Finally the jet/disk-symbiosis model, which successfully explains radio cores in LINER galaxies, is applied to the stellar mass black hole GRS 1915+105, indicating that the radio cores in both types of sources are just different sides of the same coin. The conclusion drawn from all these observations is that radio jets are a ubiquitous feature of most---if not all---AGN and play an important effect in the overall energy budget, as well as for the interpretation of observations in other wavebands (e.g. optical emission lines).

Open-access reader

About this research paper

What this paper is about

This paper summarizes some of our recent projects which try to illuminate the nature and importance of jets associated with active nuclei and compact objects. After a short introduction on jets in radio galaxies and radio loud quasars the paper focuses on jets in other source types, such as radio-quiet quasars, Seyfert and LINER galaxies, and stellar mass black holes. Radio observations of quasars, for example, have brought new evidence for the existence of relativistic jets in radio quiet quasars, while HST and VLA observations of Seyfert galaxies have now clearly established not only the presence of radio jets, but also the great importance these jets have for the morphology and the excitation of the emission line region in these AGN. Moreover, a recent VLA survey found a large fraction of low-luminosity AGN to host compact, flat-spectrum radio cores indicating the presence of radio jets there as well. Finally the jet/disk-symbiosis model, which successfully explains radio cores in LINER galaxies, is applied to the stellar mass black hole GRS 1915+105, indicating that the radio cores in both types of sources are just different sides of the same coin. The conclusion drawn from all these observations is that radio jets are a ubiquitous feature of most---if not all---AGN and play an important effect in the overall energy budget, as well as for the interpretation of observations in other wavebands (e.g. optical emission lines).

Why it matters

A significance statement is not available in the OpenAlex record.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

This paper summarizes some of our recent projects which try to illuminate the nature and importance of jets associated with active nuclei and compact objects. After a short introduction on jets in radio galaxies and radio loud quasars the paper focuses on jets in other source types, such as radio-quiet quasars, Seyfert and LINER galaxies, and stellar mass black holes. Radio observations of quasars, for example, have brought new evidence for the existence of relativistic jets in radio quiet quasars, while HST and VLA observations of Seyfert galaxies have now clearly established not only the presence of radio jets, but also the great importance these jets have for the morphology and the excitation of the emission line region in these AGN. Moreover, a recent VLA survey found a large fraction of low-luminosity AGN to host compact, flat-spectrum radio cores indicating the presence of radio jets there as well. Finally the jet/disk-symbiosis model, which successfully explains radio cores in LINER galaxies, is applied to the stellar mass black hole GRS 1915+105, indicating that the radio cores in both types of sources are just different sides of the same coin. The conclusion drawn from all these observations is that radio jets are a ubiquitous feature of most---if not all---AGN and play an important effect in the overall energy budget, as well as for the interpretation of observations in other wavebands (e.g. optical emission lines).

Key concepts: Physics, Astrophysics, Quasar, Astrophysical jet, Radio galaxy, Active galactic nucleus, Galaxy, Luminosity

Related papers

Back to paper searchBrowse research topicsOriginal source
Jets in AGN -- New Results from HST and VLA — Research Paper | ScholarLens