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Can pre-supernova winds from massive stars enrich the interstellar medium with nitrogen at high redshift?
Arpita Roy, Mark R. Krumholz, Michael A. Dopita +3
Understanding the nucleosynthetic origin of nitrogen and the evolution of the N/O ratio in the interstellar medium is crucial for a comprehensive picture of galaxy chemical evoluti…
Theoretically Modelling Photoionized Regions with Fractal Geometry in Three Dimensions
Yifei Jin, Lisa J. Kewley, Ralph S. Sutherland
We create a photoionization model embedded in the turbulent ISM by using the state-of-the-art Messenger Monte-Carlo MAPPINGS~V code (M) in conjunction with the CMFGEN stellar a…
Messenger Monte-Carlo MAPPINGS V (M^3) -- A self-consistent three-dimensional photoionization code
Yifei Jin, Lisa Kewley, Ralph Sutherland
The Messenger Interface Monte-Carlo Mappings V (M^3) is a photoionization code adopting the fully self-consistent Monte-Carlo radiative transfer technique, which presents a major a…
Modelling observable signatures of jet-ISM interaction: thermal emission and gas kinematics
Moun Meenakshi, Dipanjan Mukherjee, Alexander Y. Wagner +6
Relativistic jets are believed to have a substantial impact on the gas dynamics and evolution of the interstellar medium (ISM) of their host galaxies. In this paper, we aim to draw…