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The Dynamics and Energetics of Remnant and Restarting RLAGN
by
Mahatma, Vijay H.
in
Active galactic nuclei
/ Active galaxies
/ Astronomical research
/ Black holes
/ Galaxies
/ jets
/ Magnetic fields
/ Morphology
/ Numerical prediction
/ Numerical simulations
/ Physical properties
/ Population statistics
/ Quasars
/ Radio galaxies
/ radio galaxy lifecycles
/ Radio observation
/ radio observations
/ Restarting
/ Simulation
/ simulations
/ Star & galaxy formation
/ Stars & galaxies
/ Subpopulations
2023
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The Dynamics and Energetics of Remnant and Restarting RLAGN
by
Mahatma, Vijay H.
in
Active galactic nuclei
/ Active galaxies
/ Astronomical research
/ Black holes
/ Galaxies
/ jets
/ Magnetic fields
/ Morphology
/ Numerical prediction
/ Numerical simulations
/ Physical properties
/ Population statistics
/ Quasars
/ Radio galaxies
/ radio galaxy lifecycles
/ Radio observation
/ radio observations
/ Restarting
/ Simulation
/ simulations
/ Star & galaxy formation
/ Stars & galaxies
/ Subpopulations
2023
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Do you wish to request the book?
The Dynamics and Energetics of Remnant and Restarting RLAGN
by
Mahatma, Vijay H.
in
Active galactic nuclei
/ Active galaxies
/ Astronomical research
/ Black holes
/ Galaxies
/ jets
/ Magnetic fields
/ Morphology
/ Numerical prediction
/ Numerical simulations
/ Physical properties
/ Population statistics
/ Quasars
/ Radio galaxies
/ radio galaxy lifecycles
/ Radio observation
/ radio observations
/ Restarting
/ Simulation
/ simulations
/ Star & galaxy formation
/ Stars & galaxies
/ Subpopulations
2023
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The Dynamics and Energetics of Remnant and Restarting RLAGN
Journal Article
The Dynamics and Energetics of Remnant and Restarting RLAGN
2023
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Overview
In this article, I review past, current, and future advances on the study of radio-loud AGN (RLAGN; radio-loud quasars and radio galaxies) lifecycles exclusively in the remnant and restarting phases. I focus on their dynamics and energetics as inferred from radio observations while discussing their radiative lifetimes, population statistics, and trends in their physical characteristics. I briefly summarise multi-wavelength observations, particularly X-rays, that have enabled studies of the large-scale environments of RLAGN in order to understand their role in feedback. Furthermore, I discuss analytic and numerical simulations that predict key properties of remnant and restarting sources as found in wide-area surveys, and discuss the prospects of future surveys that may shed further light on these elusive subpopulations of RLAGN.
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