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Using Anisotropies as a Forensic Tool for Decoding Supernova Remnants

  • Authors: Abigail Polin, Paul Duffell, Dan Milisavljevic

Abigail Polin et al 2022 The Astrophysical Journal Letters 940 .

  • Provider: AAS Journals

Caption: Figure 2.

Power spectrum associated with the s = 2, n = 7 Chevalier solution. Left: velocity power spectra at different computational resolutions. The dark line tracing the data is the data smoothed via a Gaussian smoothing process used throughout the rest of this work for visualization purposes. Right: the smoothed power spectra of density (green) and velocity (purple) for the high-resolution model. Dashed lines trace the slopes of the characteristic power laws and the solid vertical line denotes the dominant mode, l 0, at which they break. The secondary peak at high l is caused by the grid scale.

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