Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Title A name given to the resource Faculty Publications Article Faculty Publications -Articles Dublin Core The Dublin Core metadata element set is common to all Omeka records, including items, files, and collections. For more information see, http://dublincore.org/documents/dces/. Creator An entity primarily responsible for making the resource Giri, Gourab; Fendt, Christian; Bagchi, Joydeep; Thorat, Kshitij; Saikia, Dhruba J.; Deane, Roger P.; Delhaize, Jacinta Title A name given to the resource Probing the formation of megaparsec-scale giant radio galaxies II. Continuum and polarization behavior from magneto-hydrodynamic simulations Date A point or period of time associated with an event in the lifecycle of the resource 01-01-2025 Source A related resource from which the described resource is derived Astronomy and Astrophysics;Volume;703;Issue;;Article No.;A214; Identifier An unambiguous reference to the resource within a given context <a href="https://doi.org/10.1051/0004-6361/202554872" target="_blank" rel="noreferrer noopener">https://doi.org/10.1051/0004-6361/202554872</a> <br /><br /><a href="https://www.scopus.com/pages/publications/105022885217?origin=resultslist" target="_blank" rel="noreferrer noopener">https://www.scopus.com/pages/publications/105022885217?origin=resultslist</a> Coverage The spatial or temporal topic of the resource, the spatial applicability of the resource, or the jurisdiction under which the resource is relevant Giri G., Istituto Nazionale di Astrofisica (INAF), Istituto di Radioastronomia (IRA), via Gobetti 101, Bologna, 40129, Italy, Department of Physics, University of Pretoria, Private Bag X20, Hatfield, 0028, South Africa; Fendt C., Max Planck Institute for Astronomy, Kigstuhl 17, Heidelberg, D-69117, Germany; Bagchi J., Department of Physics and Electronics, Christ University, Hosur Road, Bangalore, 560029, India; Thorat K., Department of Physics, University of Pretoria, Private Bag X20, Hatfield, 0028, South Africa; Saikia D.J., Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Pune, 411007, India; Deane R.P., Department of Physics, University of Pretoria, Private Bag X20, Hatfield, 0028, South Africa, Wits Centre for Astrophysics, School of Physics, University of the Witwatersrand, 1 Jan Smuts Avenue, Johannesburg, 2000, South Africa; Delhaize J., Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch, 7701, South Africa Description An account of the resource Context. The persistence of radiative signatures in giant radio galaxies (GRGs &amp; 700 kpc) remains a frontier topic of research, with contemporary telescopes revealing intricate features that require investigation. Aims. This study aims to examine the emission characteristics of simulated GRGs, and correlate them with their underlying three-dimensional dynamical properties. Methods. Sky-projected continuum and polarization maps at 1 GHz were computed from five 3D relativistic magnetohydrodynamical (RMHD) simulations by integrating the synthesized emissivity data along the line of sight, with the integration path chosen to reflect the GRG evolution in the sky plane. The emissivities were derived from these RMHD simulations, featuring FR-I and FR-II jets injected at different locations of the large-scale environment and with propagation along varying jet frustration paths. Results. Morphologies, such as widened lobes from low-power jets and collimated flows from high-power jets, are strongly shaped by the triaxiality of the environment, resulting in features such as wings and asymmetric cocoons, thereby making morphology a crucial indicator of GRG formation mechanisms. The decollimation of the bulk flow in GRG jets gives rise to intricate cocoon features, most notably filamentary structuresmagnetically dominated threads with lifespans of a few mega-year. High jet power cases frequently display enhanced emission zones at mid-cocoon distances (alongside warmspots around the jet head), contradicting the interpretations of the GRG as a restarting source. In such cases, examining the lateral intensity variation of the cocoon may reveal the sources state, with a gradual decrease in emission suggesting a low active stage. This study highlights that applying a simple radio powerjet power relation to a statistical GRG sample is unfeasible, as it depends on growth conditions of individual GRGs. Effects such as inverse-Compton cooling due to cosmic microwave background photons and matter entrainment significantly impact the long-term emission persistence of GRGs. The diminishing fractional polarization with GRG evolution reflects increasing turbulence, underscoring the importance of modeling this characteristic further, particularly for even larger-scaled sources. The Authors 2025. Subject The topic of the resource galaxies: active; galaxies: groups: general; galaxies: jets; magnetohydrodynamics (MHD); methods: numerical Publisher An entity responsible for making the resource available EDP Sciences Relation A related resource ISSN: 46361; CODEN: AAEJA Language A language of the resource English Type The nature or genre of the resource Article Rights Information about rights held in and over the resource All Open Access; Gold Open Access Format The file format, physical medium, or dimensions of the resource online