Analyzing Unusual Radio Outflows in extended RAdio-galaxies (AURORA)

Project Description:

Analyzing Unusual Radio Outflows in extended RAdio-galaxies (AURORA): In a small fraction of the extragalactic jets, an intriguing phenomenon occurs wherein the initially straight trajectory of the jet starts bending, giving rise to peculiar morphologies that appear like X-, S-, and Z-shapes or in general, “winged”-shapes. With the remarkable resolution and sensitivity of current-day telescopes, a substantial increase in the discovery of winged radio galaxies has commenced. These discoveries present an opportunity to delve into the origins of such phenomena, a topic that has long been debated. However, while observations provide valuable insights into different emission components, they often fall short in fully constraining the underlying formation processes. This is where numerical simulation becomes important. The primary goal of this project is to develop a state-of-the-art simulation framework aimed at addressing a fundamental question: Can a universal formation model for winged sources explain all observable properties, or are different models required for distinct sources? See the document attached below for full description.

Research Area:

Astrophysics

Project Level:

Masters

This Project Is Offered At The Following Node(s):

(UCT)(NWU)

Special Requirements:

Familiarity with python coding and Linux environment is a must.