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.
