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What is Dusty Star-Forming Galaxies at z~1.5 about?

This study investigates three dusty star-forming galaxies at redshift z ∼ 1.5, analyzing their merger histories and star formation rates in relation to the main sequence of galaxies. The findings suggest that two of the galaxies are merger-driven while one is an isolated disk galaxy, with varying positions relative to the main sequence. This indicates that the location of a galaxy concerning the main sequence may not reliably reflect its recent star formation history.

Author

h42qsjsjyd

Language

EN