JWST imaging of the Pleiades: Anisotropy of turbulence in the cold neutral medium

Open Access

Table 3

Power-law fits of the residual spectrum.

Mask	A_res	α_res	χ²
	(Jy² sr⁻¹)
	(a)	(b)	(c)
Fiducial	1.4 ± 0.1 × 10⁻⁵	−1.23 ± 0.025	2.8
Light	5.9 ± 0.8 × 10⁻⁵	−1.40 ± 0.056	24
Heavy	1.2 ± 0.2 × 10⁻⁵	−1.24 ± 0.060	13

Notes. (a) Amplitude of the power law at wavenumber k₀= 10⁻² pix $k_{0} = 10^{- 2}$ $Mathematical equation: $k_{0}= 10^{-2}$$ . (b) Spectral index of the power law. (c) Reduced χ² of the fit.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.