activity
20082026
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 4.9k across the 139 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.GA2015★ 175 cited

Is Turbulence in the Interstellar Medium Driven by Feedback or Gravity? An Observational Test

Mark R. Krumholz, Blakesley Burkhart

Galaxies' interstellar media (ISM) are observed to be supersonically-turbulent, but the ultimate power source that drives turbulent motion remains uncertain. The two dominant model…

physics.space-ph2015★ 12 cited

Principal Component Analysis studies of turbulence in optically thick gas

Caio Correia, Alex Lazarian, Blakesley Burkhart +2

In this work we investigate the Principal Component Analysis (PCA) sensitivity to the velocity power spectrum in high opacity regimes of the interstellar medium (ISM). For our anal…

astro-ph.GA2015★ 16 cited

The Phase Coherence of Interstellar Density Fluctuations

Blakesley Burkhart, Alex Lazarian

Studies of MHD turbulence often investigate the Fourier power spectrum to provide information on the nature of the turbulence cascade. However, the Fourier power spectrum only cont…

astro-ph.GA2015★ 57 cited

The Lognormal Probability Distribution Function of the Perseus Molecular Cloud: A Comparison of HI and Dust

Blakesley Burkhart, Min-Young Lee, Claire Murray +1

The shape of the probability distribution function (PDF) of molecular clouds is an important ingredient for modern theories of star formation and turbulence. Recently, several stud…

astro-ph.GA2015★ 59 cited

The Turbulence Velocity Power Spectrum of Neutral Hydrogen in the Small Magellanic Cloud

Alexey Chepurnov, Blakesley Burkhart, Alex Lazarian +1

We present the results of the Velocity Coordinate Spectrum (VCS) technique to calculate the velocity power spectrum of turbulence in the Small Magellanic Cloud (SMC) in 21cm emissi…

astro-ph.SR2015★ 75 cited

Observational Diagnostics of Self-Gravitating MHD Turbulence in Giant Molecular Clouds

Blakesley Burkhart, David C. Collins, Alex Lazarian

We study the observable signatures of self-gravitating MHD turbulence by applying the probability density functions (PDFs) and the spatial density power spectrum to synthetic colum…