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What is Dense Molecular Gas in High-Redshift Galaxies about?

This study investigates HCN emission in four high-redshift infrared-luminous galaxies, which are believed to be in a significant starburst phase of spheroidal galaxy formation. The research reports a marginal detection of HCN emission from one galaxy and upper limits for others, suggesting that star formation is a primary driver of infrared luminosity in these systems. The findings indicate that the HCN to far-IR luminosity ratios for these high-redshift galaxies align with those observed in lower redshift

Author

ljliu.astro

Language

EN