Faraday Discuss., 2023, 245,181-198
DOI: 10.1039/D3FD00007A, Paper
DOI: 10.1039/D3FD00007A, Paper
Ko-Yun Huang, Serena Viti
We present an astrochemical modeling study with the aim of comparing shock chemistry traced by HNCO and SiO in two distinctively different environments: the AGN dominated region in the CND of NGC 1068 and the starburst-dominated region in the CMZ of NGC 253.
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We present an astrochemical modeling study with the aim of comparing shock chemistry traced by HNCO and SiO in two distinctively different environments: the AGN dominated region in the CND of NGC 1068 and the starburst-dominated region in the CMZ of NGC 253.
The content of this RSS Feed (c) The Royal Society of Chemistry