443 citations · 4.9k across the 139 of their papers we have counts for
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Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
Philip Mocz, Blakesley Burkhart
Supersonic isothermal turbulence establishes a network of transient dense shocks that sweep up material and have a density profile described by balance between ram pressure of the…
The Self-gravitating Gas Fraction and The Critical Density for Star Formation
Blakesley Burkhart, Philip Mocz
We analytically calculate the star formation efficiency and dense self-gravitating gas fraction in the presence of magneto-gravo-turbulence using the model of Burkhart (2018), whic…
Statistical tracing of magnetic fields: comparing and improving the techniques
Ka Ho Yuen, Junda Chen, Yue Hu +9
Magnetohydrodynamic(MHD) turbulence displays velocity anisotropies which reflect the direction of the magnetic field. This anisotropy has led to the development of a number of stat…
The CARMA-NRO Orion Survey
Shuo Kong, Héctor G. Arce, Jesse R. Feddersen +35
We present the first results from a new, high resolution, CO(1-0), CO(1-0), and CO(1-0) molecular line survey of the Orion A cloud, hereafter referred to as th…
The Multi-phase Turbulence Density Power Spectra in the Perseus Molecular Cloud
Nickolas Pingel, Min-Young Lee, Blakesley Burkhart +1
We derive two-dimensional spatial power spectra of four distinct interstellar medium tracers, HI, CO(=1--0), CO(=1--0), and dust, in the Perseus molecular cloud…
Advanced Diagnostics for the Study of Linearly Polarized Emission. II: Application to Diffuse Interstellar Radio Synchrotron Emission
C. A. Herron, Blakesley Burkhart, B. M. Gaensler +8
Diagnostics of polarized emission provide us with valuable information on the Galactic magnetic field and the state of turbulence in the interstellar medium, which cannot be obtain…
The Star Formation Rate in the Gravoturbulent Interstellar Medium
Blakesley Burkhart
Stars form in supersonic turbulent molecular clouds that are self-gravitating. We present an analytic determination of the star formation rate (SFR) in a gravoturbulent medium base…