Local Volume HI Survey: the far-infrared radio correlation
Li Shao, Baerbel Koribalski, Jing Wang, Luis Ho, Lister Staveley-Smith

TL;DR
This study confirms a tight linear far-infrared radio correlation in local gas-rich galaxies, including dwarfs, and explores the underlying factors maintaining this relation despite individual deficiencies.
Contribution
It provides the first detailed analysis of the FIR-radio correlation in a volume-limited sample of local galaxies, including dwarfs, and investigates the physical factors behind the correlation's robustness.
Findings
FIR-radio correlation holds over four orders of magnitude.
Dwarf galaxies are deficient in FIR and radio emissions relative to star formation.
Multiple galaxy properties cancel out, maintaining the FIR-radio ratio.
Abstract
In this paper we measure the far-infrared (FIR) and radio flux densities of a sample of 82 local gas-rich galaxies, including 70 "dwarf" galaxies (), from the Local Volume HI Survey (LVHIS), which is close to volume limited. It is found that LVHIS galaxies hold a tight linear FIR-radio correlation (FRC) over four orders of magnitude (). However, for detected galaxies only, a trend of larger FIR-to-radio ratio with decreasing flux density is observed. We estimate the star formation rate by combining UV and mid-IR data using empirical calibration. It is confirmed that both FIR and radio emission are strongly connected with star formation but with significant non-linearity. Dwarf galaxies are found radiation deficient in both bands, when normalized by star formation rate. It urges a "conspiracy" to keep the FIR-to-radio ratio…
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