**Table 3:** Fluxes and positions for the 2 continuum peaks inferred from global fits to the uv plane data.
Source	Frequency	Wavelength	Fitted shape	Flux^a	Offset from phase center
	(GHz)	(mm)		(mJy)	('')
RW Aur A	230.5	1.30	Gaussian^b	$27.6 \pm 0.5$	$~~0.000 \pm 0.005 \times -0.067 \pm 0.007$
	112.5	2.66	Point	$~8.0 \pm 0.3$	$-0.06 \pm 0.03 \times -0.07 \pm 0.02$
RW Aur B	230.5	1.30	Point	$~5.2 \pm 0.4$	$-1.42 \pm 0.03 \times -0.44 \pm 0.04$
	112.5	2.66	Point	$~0.8 \pm 0.3$	$-1.34 \pm 0.28 \times -0.48 \pm 0.24$

^a Quoted 1- $\sigma$ flux uncertainties only reflect thermal and phase noises. The absolute flux calibration accuracy is estimated to be 20% (see text).
^b Fitting an elliptical Gaussian perpendicular to the jet instead of a circular Gaussian does not significantly change the results.

Source LaTeX | All tables | In the text