dc.contributor.author | Rihobot Hailu | |
dc.contributor.author | Tolu Biressa | |
dc.contributor.author | Menberu Mengesha | |
dc.date.accessioned | 2025-07-16T08:02:50Z | |
dc.date.available | 2025-07-16T08:02:50Z | |
dc.date.issued | 2024-06-27 | |
dc.identifier.uri | https://repository.ju.edu.et//handle/123456789/9750 | |
dc.description.abstract | AGN jet research is essential to comprehending galaxy evolution and the interac tions between supermassive black holes and their host environments. Interstellar dust in the host galaxy is frequently detected to obstruct the jets, which originate from the accretion disk encircling the central black hole. Misunderstandings of the jets’ inherent qualities result from this dust extinction substantial influence on the jets’ observed properties. By examining the influence of dust grain size and utilizing general relativistic hydrodynamic radiative transfer equations (RTE), This work ex plores the role of dust grain size and radiative transfer effects in galactic interstellar dust extinction and how they affect the jets that are released from AGN. We simulate the absorption and scattering of the jets using a radiative transfer model that takes into account a variety of dust grain sizes and compositions. Our findings indicate that dust extinction has a major impact on the jet properties that are observed. | en_US |
dc.language.iso | en | en_US |
dc.title | Galactic interstellar dust extinction effect on jets Emitted from galactic nuclei | en_US |
dc.type | Thesis | en_US |