Jets of collimated particles are among the most intriguing characteristics of active galactic nuclei. In this paper two models of particle interactions in active galactic nuclei are used to explore a possible initial acceleration mechanism of the jets: charge separation. Model I ignores the effects of both collisions and electromagnetic forces and does not predict charge separation. Model II incorporates collisions and electromagnetic interactions, and, although it too predicts no charge separation, it provides a more physically sound model of active nucleus than does Model I
Active Galactic Nuclei (henceforth AGN) have been observed assiduously, throughout the electromagnet...
This paper summarizes extensive observational studies of the closest ultraluminous radio galaxy Cygn...
© The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society...
The idea that galaxy interactions and merging are related to the generation of starburst and AGN act...
Jets in active galactic nuclei (AGN) are very interdisciplinary laboratories, and still as enigmatic...
This paper examines the relationship between the accretion flows into the accretion disk around the ...
Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Bec...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.Galactic-scale outflows...
Item does not contain fulltextThe radio galaxy 3C 75 is remarkable because it contains a pair of rad...
Active Galactic Nuclei (AGN) feedback is a key ingredient in galaxy formation and evolution. A large...
In the past, extragalactic radio jets have been modelled as interacting with a smooth, hot interstel...
Context. Radio-loud active galactic nuclei (AGNs) are thought to possess various sites of particle a...
Highly collimated supersonic jets and less collimated outflows are observed to emerge from a wide va...
ABSTRACT It is still a mystery why only a small fraction of active galactic nuclei (AGNs) contain re...
The phenomenology of jets associated with a variety of black hole systems is summarized, emphasizing...
Active Galactic Nuclei (henceforth AGN) have been observed assiduously, throughout the electromagnet...
This paper summarizes extensive observational studies of the closest ultraluminous radio galaxy Cygn...
© The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society...
The idea that galaxy interactions and merging are related to the generation of starburst and AGN act...
Jets in active galactic nuclei (AGN) are very interdisciplinary laboratories, and still as enigmatic...
This paper examines the relationship between the accretion flows into the accretion disk around the ...
Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Bec...
Ph.D. University of Hawaii at Manoa 2014.Includes bibliographical references.Galactic-scale outflows...
Item does not contain fulltextThe radio galaxy 3C 75 is remarkable because it contains a pair of rad...
Active Galactic Nuclei (AGN) feedback is a key ingredient in galaxy formation and evolution. A large...
In the past, extragalactic radio jets have been modelled as interacting with a smooth, hot interstel...
Context. Radio-loud active galactic nuclei (AGNs) are thought to possess various sites of particle a...
Highly collimated supersonic jets and less collimated outflows are observed to emerge from a wide va...
ABSTRACT It is still a mystery why only a small fraction of active galactic nuclei (AGNs) contain re...
The phenomenology of jets associated with a variety of black hole systems is summarized, emphasizing...
Active Galactic Nuclei (henceforth AGN) have been observed assiduously, throughout the electromagnet...
This paper summarizes extensive observational studies of the closest ultraluminous radio galaxy Cygn...
© The Author(s), 2023. Published by Cambridge University Press on behalf of the Astronomical Society...