Special Relativistic Imaging of Model Astrophysical Jets

Authors

  • Theodoros Smponias Directorate of Primary Education of the Ionian Islands, Corfu, Greece.

DOI:

https://doi.org/10.9734/bpi/cppsr/v5/8281A

Keywords:

Jets and outflows, winds-outflows, flare, radiation mechanisms, numerical

Abstract

Imaging an astrophysical object traveling at relativistic speeds, leads to a number of image distortions. These effects may be studied within the framework of a numerical simulation. In this work, a special relativistic imaging algorithm is implemented. The resulting code works together with a hydrodynamic astrophysical program, producing synthetic images, depicting what a model relativistic astrophysical jet looks like to a stationary observer. The software is able to visualize a variety of dynamical astrophysical phenomena. A number of tests are performed, in order to confirm code integrity, and to present features of the software. The above demonstrate the potential of the computer program to help interpret astrophysical jet observations.

Published

2024-01-01

How to Cite

Theodoros Smponias. (2024). Special Relativistic Imaging of Model Astrophysical Jets. Current Perspective to Physical Science Research Vol. 5, 128–162. https://doi.org/10.9734/bpi/cppsr/v5/8281A