How Plasma Properties of the Fanaroff-Riley Jet can Shape its Morphology
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2026
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| author | Tripathi, Priyesh Kumar Chattopadhyay, Indranil Joshi, Raj Kishor Chatterjee, Ritaban Debnath, Sanjit Khan, M. Saleem |
| author_facet | Tripathi, Priyesh Kumar Chattopadhyay, Indranil Joshi, Raj Kishor Chatterjee, Ritaban Debnath, Sanjit Khan, M. Saleem |
| contents | 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 (3D-MHD) 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. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2601_09349 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | How Plasma Properties of the Fanaroff-Riley Jet can Shape its Morphology Tripathi, Priyesh Kumar Chattopadhyay, Indranil Joshi, Raj Kishor Chatterjee, Ritaban Debnath, Sanjit Khan, M. Saleem High Energy Astrophysical Phenomena 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 (3D-MHD) 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. |
| title | How Plasma Properties of the Fanaroff-Riley Jet can Shape its Morphology |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2601.09349 |