Star Formation and Molecular Gas Diagnostics with Mid- and Far-infrared Emission

Star Formation and Molecular Gas Diagnostics with Mid- and Far-infrared Emission

With the start of JWST observations, mid-infrared (MIR) emission features from polycyclic aromatic hydrocarbons (PAHs), H _2 rotational lines, fine structure lines from ions, and dust continuum will be widely available tracers of gas and star formation rate (SFR) in galaxies at various redshifts. Ma...

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Bibliographic Details
Main Authors:	C. M. Whitcomb, K. Sandstrom, A. Leroy, J.-D. T. Smith
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Series:	The Astrophysical Journal
Subjects:	Molecular gas Polycyclic aromatic hydrocarbons Star forming regions Star formation
Online Access:	https://doi.org/10.3847/1538-4357/acc316

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