Table 2: Radio detections as a function of wavelength of our targets reported in the literature. When several measurements are available a weighted average is shown; upper limits are 3 $\sigma$ . Fluxes are from [1] Abbott et al. (1980), [2] Bieging et al. (1989), [3] Drake (1990), [4] Lamers & Leitherer (1993) and [5] Scuderi et al. (1998).
Star Flux (mJy)

2 cm 3.6 cm 6 cm References

$\alpha$ Cam $0.65\pm0.13$ $0.44\pm0.04$ $0.29 \pm 0.04$ 2,5

15 Mon <0.4 $0.40 \pm 0.13$ 3

<0.33 and <0.18 2,3

$\lambda$ Cep $0.38 \pm 0.03$ $0.40 \pm 0.25$ 1,4

**Table 2:** Radio detections as a function of wavelength of our targets reported in the literature. When several measurements are available a weighted average is shown; upper limits are 3 $\sigma$ . Fluxes are from [1] Abbott et al. (1980), [2] Bieging et al. (1989), [3] Drake (1990), [4] Lamers & Leitherer (1993) and [5] Scuderi et al. (1998).
Star	Flux (mJy)
	2 cm	3.6 cm	6 cm	References
$\alpha$ Cam	$0.65\pm0.13$	$0.44\pm0.04$	$0.29 \pm 0.04$	2,5
15 Mon	<0.4		$0.40 \pm 0.13$	3
			<0.33 and <0.18	2,3
$\lambda$ Cep		$0.38 \pm 0.03$	$0.40 \pm 0.25$	1,4

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