How Plasma Properties of the Fanaroff–Riley Jet Can Shape Its Morphology

Abstract Extragalactic jets are broadly classified into two categories based on radio observations: core-brightened jets, known as Fanaroff–Riley Type I (FR I), and edge-brightened jets, classified as Type II (FR II). This FR dichotomy may arise due to variation in the ambient medium and/or the properties of the jet itself, such as injection speed, temperature, composition, magnetization, etc. To investigate this, we perform large-scale three-dimensional magnetohydrodynamic simulations of low-power, supersonic jets extending to kiloparsec scales. We inject a jet beam carrying an initially toroidal magnetic field into a denser, unmagnetized, and stratified ambient medium through a cylindrical nozzle. Our simulations explore jets with varying injection parameters to investigate their impact on morphology and emission properties. Furthermore, we examine jets with significantly different plasma compositions, such as hadronic and mixed electron–positron–proton configurations, to study the conditions that may drive transitions between FR I and FR II morphologies. We find that, under the same injection parameters, mixed plasma composition jets tend to evolve into FR I structures. In contrast, electron–proton jets exhibit a transition between FR I and FR II morphologies at different stages of their evolution.

Authors

Publication Details

Journal
The Astrophysical Journal
Published
2026-02-13
DOI
https://doi.org/10.3847/1538-4357/ae38e2
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
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article

How Plasma Properties of the Fanaroff–Riley Jet Can Shape Its Morphology

Priyesh Kumar Tripathi, Indranil Chattopadhyay, Ritaban Chatterjee, Raj Kishor Joshi et al.
The Astrophysical Journal
Astrophysics and Cosmic Phenomena
article

How Plasma Properties of the Fanaroff–Riley Jet Can Shape Its Morphology

Priyesh Kumar Tripathi, Indranil Chattopadhyay, Ritaban Chatterjee, Raj Kishor Joshi, M. Saleem Khan, Sanjit Debnath
article en

Abstract

Abstract Extragalactic jets are broadly classified into two categories based on radio observations: core-brightened jets, known as Fanaroff–Riley Type I (FR I), and edge-brightened jets, classified as Type II (FR II). This FR dichotomy may arise due to variation in the ambient medium and/or the properties of the jet itself, such as injection speed, temperature, composition, magnetization, etc. To investigate this, we perform large-scale three-dimensional magnetohydrodynamic simulations of low-power, supersonic jets extending to kiloparsec scales. We inject a jet beam carrying an initially toroidal magnetic field into a denser, unmagnetized, and stratified ambient medium through a cylindrical nozzle. Our simulations explore jets with varying injection parameters to investigate their impact on morphology and emission properties. Furthermore, we examine jets with significantly different plasma compositions, such as hadronic and mixed electron–positron–proton configurations, to study the conditions that may drive transitions between FR I and FR II morphologies. We find that, under the same injection parameters, mixed plasma composition jets tend to evolve into FR I structures. In contrast, electron–proton jets exhibit a transition between FR I and FR II morphologies at different stages of their evolution.

The Astrophysical JournalVol. 998(2)
Openalex Percentile: Top 53%
Astrophysics and Cosmic Phenomena
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