Effect of OH depletion on measurements of the mass-to-flux ratio in molecular cloud cores
K. Tassis, K. Willacy, H. W. Yorke, N. J. Turner

TL;DR
This paper investigates how chemical depletion of OH affects the accuracy of mass-to-flux ratio measurements in molecular cloud cores, revealing potential errors and trend reversals in magnetic and gravitational force assessments.
Contribution
It demonstrates that OH depletion causes significant systematic errors in mass-to-flux ratio measurements, challenging previous assumptions of constant abundance across regions.
Findings
OH depletion can reverse the apparent trend of mass-to-flux ratio with density.
Systematic errors mainly stem from inaccurate mass estimations due to depletion.
Assuming constant OH abundance across regions is invalid, affecting magnetic field measurements.
Abstract
The ratio of mass and magnetic flux determines the relative importance of magnetic and gravitational forces in the evolution of molecular clouds and their cores. Its measurement is thus central in discriminating between different theories of core formation and evolution. Here we discuss the effect of chemical depletion on measurements of the mass-to-flux ratio using the same molecule (OH) both for Zeeman measurements of the magnetic field and the determination of the mass of the region. The uncertainties entering through the OH abundance in determining separately the magnetic field and the mass of a region have been recognized in the literature. It has been proposed however that, when comparing two regions of the same cloud, the abundance will in both cases be the same. We show that this assumption is invalid. We demonstrate that when comparing regions with different densities, the…
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