Predicting interstellar radiation fields from chemical evolution models
Mario Romero, Pablo Corcho-Caballero, Iker Mill\'an-Irigoyen, Mercedes, Moll\'a, Yago Ascasibar

TL;DR
This paper introduces a new method combining chemical evolution models with radiative transfer to predict the interstellar radiation field across a broad spectrum, validated against simulations and consistent with empirical data.
Contribution
The authors develop Mixclask, a novel tool integrating Cloudy and Skirt for self-consistent ISRF predictions from chemical evolution models.
Findings
Mixclask agrees with Cloudy in test scenarios.
Models broadly match empirical ISRF data, underestimating mid-infrared emission.
Significant UV differences between models highlight new insights.
Abstract
We present a self-consistent prediction of the interstellar radiation field (ISRF), from the extreme ultraviolet (EUV) to sub-mm range, based on two chemical evolution models of a Milky Way-like galaxy (MWG). To this end, we develop a new tool called Mixclask to include gas emission, absorption and scattering from the photoionization code Cloudy into the Monte Carlo radiative transfer code Skirt. Both algorithms are invoked iteratively, until the physical properties of the ISM converge. We have designed a first test, reminiscent of a HII region, and we find that the results of Mixclask are in good agreement with a spherically symmetric Cloudy simulation. Both MWG models based on chemical evolution codes give results broadly consistent with previous empirical models reported in the literature for the ISRF of our Galaxy, albeit they systematically underestimate the mid-infrared emission.…
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Code & Models
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Taxonomy
TopicsPhotocathodes and Microchannel Plates · Atmospheric Ozone and Climate · Galaxies: Formation, Evolution, Phenomena
