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Commonalities in Strong Line Emitters

Presentation #102.01 in the session “Emission Line Galaxies in the Low Redshift Universe (Meeting-in-a-Meeting)”.

Published onJun 18, 2021
Commonalities in Strong Line Emitters

Nebular emission lines are used to diagnose physical conditions such as temperatures, gas pressure, and abundances, as well as distinguishing radiation from star-formation and from black holes. Much of this comes from spectroscopy, but in order to identify emission line galaxies, one often needs narrow-band surveys or slitless spectroscopy. Without such techniques, many of these galaxies — which are often faint and low mass — would be missed or overlooked. I will discuss commonalities in the properties of emission line galaxies found at different redshifts.


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