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Table 2

Gaussian models for the calibrated visibilities of VLBA 43 GHz and GMVA 86 GHz data.

Epoch Component S ± σS a r ± σr b PA ± σPA b a ± σa c
(mJy) (mas) (deg) (mas)

2012 Feb. 12d Core 188 ± 19.4 ... ... 0.11 ± 0.05
NE 73 ± 8.6 0.14 ± 0.01 68.5 ± 4.6 0.18 ± 0.02
C3 83 ± 9.5 0.15 ± 0.03 161.9 ± 16.7 0.04 ± 0.09
C2 10 ± 4.7 0.54 ± 0.05 156.5 ± 4.8 0.21 ± 0.05
C1 54 ± 7.0 1.13 ± 0.11 159.7 ± 3.9 0.73 ± 0.22
2012 Mar. 16d Core 106 ± 11.1 ... ... 0.09 ± 0.06
NE 98 ± 11.1 0.11 ± 0.01 51.8 ± 6.4 0.21 ± 0.03
C3 77 ± 8.4 0.11 ± 0.03 156.4 ± 15.8 0.04 ± 0.06
C2 24 ± 4.1 0.48 ± 0.03 155.8 ± 3.6 0.33 ± 0.06
C1 43 ± 5.4 1.10 ± 0.15 156.0 ± 7.4 0.85 ± 0.30
2012 May 06d Core 335 ± 33.8 ... ... 0.17 ± 0.06
NE 15 ± 5.1 0.27 ± 0.02 20.1 ± 3.9 ...
NE 25 ± 5.4 0.27 ± 0.01 109.1 ± 3.1 0.06 ± 0.03
C3 50 ± 6.9 0.15 ± 0.04 167.5 ± 14.5 ...
C1 17 ± 5.1 1.11 ± 0.04 160.7 ± 2.1 0.14 ± 0.08
2012 Jun. 11d Core 353 ± 35.5 ... ... 0.14 ± 0.07
NE 15 ± 3.9 0.29 ± 0.03 45.6 ± 5.0 ...
NE 11 ± 3.8 0.35 ± 0.02 105.9 ± 2.8 ...
C2 33 ± 4.9 0.45 ± 0.03 153.4 ± 2.8 0.34 ± 0.05
C1 18 ± 4.0 1.17 ± 0.05 161.3 ± 1.3 0.26 ± 0.14
2013 Jan. 18d Core 130 ± 13.4 ... ... 0.06 ± 0.05
NE 88 ± 9.4 0.09 ± 0.02 19.6 ± 11.6 0.21 ± 0.04
C2 17 ± 3.7 0.45 ± 0.03 150.6 ± 4.2 0.16 ± 0.07
C1 21 ± 3.9 1.08 ± 0.10 154.5 ± 0.10 0.51 ± 0.20
2013 Feb. 15d Core 148 ± 15.2 ... ... 0.07 ± 0.05
NE 109 ± 11.6 0.12 ± 0.02 22.0 ± 7.4 0.26 ± 0.03
C2 17 ± 4.2 0.42 ± 0.03 153.5 ± 4.4 0.16 ± 0.06
C1 53 ± 6.6 1.05 ± 0.25 148.7 ± 10.8 0.97 ± 0.04

2012 May 19e Core 235 ± 71.4 ... ... 0.06 ± 0.05
NE 228 ± 69.2 0.11 ± 0.02 49.3 ± 19.2 0.67 ± 0.04
SE 23 ± 12.8 0.75 ± 0.02 155.8 ± 3.3 0.07 ± 0.04
SE 45 ± 17.2 1.28 ± 0.02 159.5 ± 2.0 0.17 ± 0.05

Notes.

(a)

Flux density and estimated errors.

(b)

r and PAs are the polar coordinates of the component’s center with respect to the core. The PAs are measured from north through east. σr are estimated errors in the component position. σPA are estimated errors in the PA of the component.

(c)

The FWHM of the radius of the circular Gaussian component and estimated errors in the component size.

(d)

The VLBA 43 GHz data.

(e)

The GMVA 86 GHz data.

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