Revisiting the Integrated Star Formation Law. II. Starbursts and the Combined Global Schmidt Law
Robert C. Kennicutt Jr., Mithi A.C. de los Reyes

TL;DR
This study re-examines the star formation law in galaxies, revealing a potential bimodal behavior between starburst and non-starburst galaxies, with a consistent power-law slope of about 1.5 for the combined data.
Contribution
It demonstrates that the global star formation law may be bimodal, with different relations for starbursts and non-starbursts, challenging the previous single power-law assumption.
Findings
The combined Schmidt law fits a single power law with slope ~1.5.
Starburst and non-starburst galaxies show different slopes and offsets.
Systematic biases unlikely to explain the observed offset.
Abstract
We compile observations of molecular gas contents and infrared-based star formation rates (SFRs) for 112 circumnuclear star forming regions, in order to re-investigate the form of the disk-averaged Schmidt surface density star formation law in starbursts. We then combine these results with total gas and SFR surface densities for 153 nearby non-starbursting disk galaxies from de los Reyes \& Kennicutt (2019), to investigate the properties of the combined star formation law, following Kennicutt (1998; K98). We confirm that the combined Schmidt law can be fitted with a single power law with slope (including fitting method uncertainties), somewhat steeper than the value found by K98. Fitting separate power laws to the non-starbursting and starburst galaxies, however, produces very different slopes ( and , respectively), with a…
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