A cautionary note about composite Galactic star formation relations
Genevieve Parmentier (ARI/ZAH)

TL;DR
This paper highlights the differences between local and global star formation relations in molecular clouds and clumps, emphasizing the need for caution when interpreting composite relations due to their different measurement scales.
Contribution
It clarifies the distinction between local and global star formation relations and warns against misinterpreting their differences as changes in star formation physics.
Findings
Local and global SF relations have different slopes.
Global relations are based on ensemble averages of clumps.
Misinterpreting composite relations can lead to incorrect physical conclusions.
Abstract
We explore the pitfalls which affect the comparison of the star-formation (SF) relation for nearby molecular clouds with that for distant compact molecular clumps. We show that both relations behave differently in the (, ) space, where and are, respectively, the gas and SF rate surface densities, even when the physics of star formation is the same. This is because the SF relation of nearby clouds relates gas and star surface densities measured locally, that is, within a given interval of gas surface density, or at a given protostar location. We refer to such measurements as local measurements, and the corresponding SF relation as the local relation. In contrast, the stellar content of a distant molecular clump remains unresolved. Only the mean SF rate can be obtained from e.g. the clump infrared luminosity. One clump therefore…
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