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Table 2

Gaussian fit to the continuum emission in the two nuclei.

Sky freq. Rest freq. α J2000 , δ J2000 Convolved size Deconv. size Peak flux Peak Tba Int. flux
(GHz) (GHz) 15h34m,23°30′ () () (mJy beam-1) (K) (mJy)

Western nucleus
247.0 251.5 57.226s, 11.52′′ 0.65 × 0.44 (5) 0.22 × 0.18 (1) 132.0 (1.0) 80 153.2 (1.2)
263.1 267.9 57.226s, 11.52′′ 0.63 × 0.43 (4) 0.22 × 0.19 (2) 159.7 (1.2) 80 189.3 (1.5)
336.9 343.0 57.223s, 11.53′′ 0.54 × 0.46 (155) 0.32 × 0.16 (133) 259.0 (2.9) 70 348.4 (3.8)
347.9 354.2 57.223s, 11.53′′ 0.53 × 0.46 (155) 0.32 × 0.16 (132) 283.1 (3.1) 80 384.2 (4.2)
Eastern nucleus
247.0 251.5 57.296s, 11.36′′ 0.70 × 0.47(12) 0.36 × 0.22(32) 48 (1.0) 17 64.0 (1.3)
263.1 267.9 57.296s, 11.37′′ 0.69 × 0.46(12) 0.38 × 0.23(31) 58 (1.2) 16 80.5 (1.7)
336.9 343.0 57.293s, 11.38′′ 0.59 × 0.51(177) 0.38 × 0.31(161) 103 (2.9) 15 171.1 (4.7)
347.9 354.2 57.293s, 11.38′′ 0.58 × 0.51(178) 0.36 × 0.32(155) 115 (3.1) 15 191.6 (5.1)

Notes.Results from the double Gaussian profile fits to the continuum emission in the image plane.

(a)

Peak brightness temperatures as described in Wilson et al. (2014) and taking 81, 77, 58, and 56 K/Jy conversion factors for 247.0, 263.1, 336.9, and 347.9 GHz, respectively.

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