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

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Authors: Priyesh Kumar Tripathi, Indranil Chattopadhyay, Raj Kishor Joshi, Ritaban Chatterjee, Sanjit Debnath, M. Saleem Khan
Cited by: 1
References: 73

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.

Fields of Study & Subjects

Astrophysics and Cosmic Phenomena Solar and Space Plasma Dynamics Dust and Plasma Wave Phenomena

Publication details

Journal / source
The Astrophysical Journal
Publisher
American Astronomical Society
Volume
998
Issue
2
Pages
246–246
Publication date
13 February 2026
Language
EN