The circumstellar environment around the extreme Galactic red supergiant NML Cygni: Dense, dusty, and asymmetric

Open Access

Table 1

Properties of the continuum observations.

ν (GHz)	θ (mas × mas)	PA (°)	σ (mJy beam⁻¹)	MRS (″)
218.15	420 × 310	4.5	0.5	8.85
233.75	384 × 274	−0.8	0.5	8.27

Notes. Columns list the reference frequency, ν, for each sideband, the size of the synthesised beam, θ, and its position angle, PA, the rms noise, σ, and the maximum recoverable scale MRS of the observations.

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