dc.contributor.advisor | Prescott, M | |
dc.contributor.advisor | Santos, M | |
dc.contributor.author | Ella, Moloko Malebo | |
dc.date.accessioned | 2021-04-22T10:40:14Z | |
dc.date.available | 2021-04-22T10:40:14Z | |
dc.date.issued | 2021 | |
dc.identifier.uri | http://hdl.handle.net/11394/8224 | |
dc.description | >Magister Scientiae - MSc | en_US |
dc.description.abstract | Radio galaxies are some of the most unusual and powerful objects in the Universe
and are therefore vital for so many reasons. Studies of Radio-Loud Active
Galactic Nuclei (AGN) gives us the potential to enhance our understanding
of the key processes leading to the ejection of material, connection to the central
engine and how the jets are launched. Besides, the energetic input of
these sources is thought to have an impact in the star formation history and
properties of the ISM and ICM; thus by studying them, we can improve our
understanding of their formation, evolution and their environment. | en_US |
dc.language.iso | en | en_US |
dc.publisher | University of Western Cape | en_US |
dc.subject | Radio sources | en_US |
dc.subject | Radio galaxies | en_US |
dc.subject | Energy | en_US |
dc.subject | Morphology | en_US |
dc.title | An investigation into the morphology of radio sources | en_US |
dc.rights.holder | University of Western Cape | en_US |