The scaleheight of NGC 1058 measured from its H<scp>i</scp> power spectrum

Abstract

Abstract We have measured the H i power spectrum of the nearly face-on spiral galaxy NGC 1058 from radio-interferometric observations using a visibility based estimator. The power spectrum is well fitted by two different power laws P(U) =AUα, one with α=−2.5 ± 0.6 at small length-scales (600 pc to 1.5 kpc) and another with α=−1.0 ± 0.2 at large length-scales (1.5–10.0 kpc). We interpret this change in the slope of the power spectrum as a transition from 3D turbulence at small length-scales to 2D turbulence in the plane of the galaxy's disc at large length-scales. We use the observed break in the power spectrum to estimate the galaxy's scaleheight, which we find to be 490 ± 90 pc.