Angular power spectrum of supernova remnants: effects of structure, geometry and diffuse foreground

Abstract

The study of the intensity fluctuation power spectrum of individual supernova remnants (SNRs) can reveal the structures present at sub-pc scales, and also constrain the physical process that generates those structures. There are various effects, such as the remnant shell thickness, projection of a three-dimensional structure onto a two-dimensional observational plane, and the presence of diffuse "foreground" emission, which causes the observed power spectrum to deviate from the intrinsic power spectrum of the fluctuations. Here, we report results from a systematic study of these effects, using direct numerical simulations, in the measured power spectrum. For an input power-law power spectrum, independent of the power-law index, we see a break in the observed power law at a scale which depends on the shell thickness of a shell-type SNR, and the three-dimensional turbulence changes to two-dimensional turbulence beyond that scale. We also report how the estimated power spectrum is expected to deviate from the intrinsic SNR power spectrum in the presence of additional diffuse Galactic synchrotron emission (DGSE) around the remnant shell. For a reasonable choice of the parameters, if the intrinsic SNR power spectrum is shallower than the DGSE power spectrum, the SNR contribution dominates at small angular scales of the estimated power spectra. On the other hand, if the SNR power spectrum is relatively steeper, the original power spectra is recovered only over a small window of angular scales. This study shows how detailed modeling may be used to infer the true power spectrum from the observed SNR intensity fluctuations power spectrum, which in turn can be used to constrain the nature of the turbulence that gives rise to these small scale structures.

arXiv comment8 pages, 5 figures, Accepted for publication in MNRAS

References in corpus (10)

• Modelling the supernova-driven ISM in different environments
• Modeling SNR Cassiopeia A from the Supernova Explosion to its Current Age: The role of post-explosion anisotropies of ejecta
• Supernova Remnants Interacting with Molecular Clouds: X-ray and Gamma-ray Signatures
• Visibility based angular power spectrum estimation in low frequency radio interferometric observations
• Are Models for Core-Collapse Supernova Progenitors Consistent with the Properties of Supernova Remnants?
• The visibility based Tapered Gridded Estimator (TGE) for the redshifted 21-cm power spectrum
• Numerical simulations of supernova remnants in turbulent molecular clouds
• Detailed study of the ELAIS N1 field with the uGMRT - I. Characterizing the 325 MHz foreground for redshifted 21 cm observations
• A study of Kepler supernova remnant: angular power spectrum estimation from radio frequency data
• Numerically investigating the morphology of the supernova remnant SN 1006 in the ambient medium with a density discontinuity

Cited by in corpus (1)

• The auto and cross angular power spectrum of the Cas A supernova remnant in radio and X-ray