Tracing the chemical footprint of shocks in AGN-host and starburst galaxies with ALMA multi-line molecular studies

Ko-Yun Huang; Serena Viti

doi:10.1039/d3fd00007a

Tracing the chemical footprint of shocks in AGN-host and starburst galaxies with ALMA multi-line molecular studies

Faraday Discuss. 2023 Sep 20;245(0):181-198. doi: 10.1039/d3fd00007a.

Authors

Ko-Yun Huang¹, Serena Viti^{1

2}

Affiliations

¹ Leiden Observatory, Leiden University, PO Box 9513, NL-2300 RA Leiden, The Netherlands. kyhuang@strw.leidenuniv.nl.
² Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK.

PMID: 37381784
DOI: 10.1039/d3fd00007a

Abstract

Multi-line molecular observations are an ideal tool for a systematic study of the physico-chemical processes in the Interstellar Medium (ISM), given the wide range of critical densities associated with different molecules and their transitions, and the dependencies of chemical reactions on the energy budget of the system. Recently high spatial resolution of typical shock tracers - SiO, HNCO, and CH₃OH - have been studied in the potentially shocked regions in two nearby galaxies: NGC 1068 (an AGN-host galaxy) (Huang et al., Astron. Astrophys., 2022, 666, A102; Huang et al., in prep.) and NGC 253 (a starburst galaxy) (K.-Y. Huang et al., arXiv, 2023, preprint, arXiv:2303.12685, DOI: 10.48550/arXiv.2303.12685). This paper is dedicated to the comparative study of these two distinctively different galaxies, with the aim of determining the differences in their energetics and understanding large-scale shocks in different types of galaxies.