A model for line absorption and emission from turbulent mixing layers. Issue 1 (24th August 2021)

• Record Type: Journal Article
• Authors: Tan, Brent; Oh, S Peng
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 508:Issue 1(2021)
• Page Start: L37
• Page End: L42
• Publication Date: 2021-08-24
• Subjects: hydrodynamics -- instabilities -- turbulence -- galaxies: clusters: general -- galaxies: evolution -- galaxies: haloes; Astronomy -- Research -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnrasl/slab100
• Languages: English
• ISSNs: 1745-3933

Abstract

ABSTRACT: Turbulent mixing layers (TMLs) are ubiquitous in multiphase gas. They can potentially explain observations of high ions such as O vi, which have significant observed column densities despite short cooling times. Previously, we showed that global mass, momentum, and energy transfer between phases mediated by TMLs is not sensitive to details of thermal conduction or numerical resolution. By contrast, we show here that observables such as temperature distributions, column densities, and line ratios are sensitive to such considerations. We explain the reason for this difference. We develop a prescription for applying a simple 1D conductive-cooling front model which quantitatively reproduces 3D hydrodynamic simulation results for column densities and line ratios, even when the TML has a complex fractal structure. This enables subgrid absorption and emission line predictions in large scale simulations. The predicted line ratios are in good agreement with observations, while observed column densities require numerous mixing layers to be pierced along a line of sight.