**Table 2:** Positions, millimeter flux densities, sizes, and masses of the cores detected in L1206.
	Position
	$\alpha({\rm J2000})$	$\delta({\rm J2000})$	$I^{\rm peak}_\nu$ (2.7mm)^a	$S_\nu$ (2.7mm)^b	$\theta^c$	Mass^d	$n({\rm H_2})^e$	$N({\rm H_2})^e$
Core	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	(mJy beam^-1)	(mJy)	(arcsec)	( $M_{\odot}$ )	(cm^-3)	(cm^-2)
OVRO 1	22 28 50.49	+64 13 50.7	$\phantom{2} 6.8 \pm 1.4$	$\phantom{1} 9.8 \pm2.0$	9.3	1.6	$6.5\times10^5$	$5.5\times10^{22}$
OVRO 2^f	22 28 51.41	+64 13 41.1	$\phantom{1} 59.2\pm11.8$	$\phantom{1} 86.0\pm17.2$	3.5	$14.2\phantom{1}$	$1.1\times10^8$	$3.4\times10^{24}$
OVRO 3	22 28 53.25	+64 13 32.1	$10.9\pm2.2$	$11.0\pm2.2$	5.4	1.8	$3.7\times10^6$	$1.8\times10^{23}$
OVRO 4	22 28 53.98	+64 13 34.5	$10.7\pm2.1$	$13.0\pm2.6$	5.6	2.2	$4.0\times10^6$	$2.0\times10^{23}$

^a Peak intensity corrected for primary beam response. The uncertainty in the values of the flux density is $\sim$ 20%.
^b Integrated flux density corrected for primary beam response. The uncertainty in the values of the flux density is $\sim$ 20%.
^c Deconvolved geometrical mean of the major and minor axes of the half-peak intensity contour.
^d Total (gas+dust) circumstellar mass, obtained assuming a dust temperature of 33 K (see Sect. 4.1).
^e Average H₂ volume and column density estimated assuming spherical symmetry and a mean molecular mass per H₂ molecule of $2.8m_{\rm H}$ .
^f Associated with IRAS 22272+6358A.

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