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|Abstract:||We explore the self-regulation of star formation using a large suite of high-resolution hydrodynamic simulations, focusing on molecule-dominated regions (galactic centers and [U]LIRGS) where feedback from star formation drives highly supersonic turbulence. In equilibrium, the total midplane pressure, dominated by turbulence, must balance the vertical weight of the interstellar medium. Under self-regulation, the momentum flux injected by feedback evolves until it matches the vertical weight. We test this flux balance in simulations spanning a wide range of parameters, including surface density Σ, momentum injected per stellar mass formed (p */m *), and angular velocity. The simulations are two-dimensional radial-vertical slices, and include both self-gravity and an external potential that helps to confine gas to the disk midplane. After the simulations reach a steady state in all relevant quantities, including the star formation rate Σ SFR, there is remarkably good agreement between the vertical weight, the turbulent pressure, and the momentum injection rate from supernovae. Gas velocity dispersions and disk thicknesses increase with p */m *. The efficiency of star formation per free-fall time at the midplane density, εff(n 0), is insensitive to the local conditions and to the star formation prescription in very dense gas. We measure εff(n 0) 0.004-0.01, consistent with low and approximately constant efficiencies inferred from observations. For Σ ∈ (100-1000) M pc-2, we find ΣSFR ∈ (0.1-4) M kpc-2 yr-1, generally following a ΣSFR Σ2 relationship. The measured relationships agree very well with vertical equilibrium and with turbulent energy replenishment by feedback within a vertical crossing time. These results, along with the observed Σ-ΣSFR relation in high-density environments, provide strong evidence for the self-regulation of star formation. © 2012. The American Astronomical Society. All rights reserved.|
|Electronic Publication Date:||27-Jun-2012|
|Citation:||Shetty, R, Ostriker, EC. (2012). Maximally star-forming galactic disks. II. vertically resolved hydrodynamic simulations of starburst regulation. Astrophysical Journal, 754 (1), 10.1088/0004-637X/754/1/2|
|Type of Material:||Journal Article|
|Journal/Proceeding Title:||Astrophysical Journal|
|Version:||Final published version. Article is made available in OAR by the publisher's permission or policy.|
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