Correlation between accretion rate and free-free emission in protoplanetary disks - A multiwavelength analysis of central mm/cm emission in transition disks

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Table 5

Estimated inner disk dust mass.

Target	Band	Beam size	R_id (au)	M_dust (M_⊕)
GG Tau	Band 7	0.″195 × 0.″135	<30	~1.00
HD 100546	Band 6	0.″025 × 0.″017	<1.9	~0.024
HD 142527	Band 7	0.″139 × 0..″120	<18.8	~0.096
AB Aur	Band 6	0.″040 × 0.″022	<6.5	~0.022
HD100453	Band 7	0.″035 × 0.″031	<3.6	~0.011
WSB60	Band 6	0.″048 × 0.″030	<4.1	~1.37
HD 169142	Band 6	0.″072 × 0.″043	<4.9	~0.0076
HD 135344B	Band 6	0.″245 × 0.″180	<24.5	~0.013
MWC758	Band 7	0.″040 × 0.″031	<5.0	~0.0042
SR24S	Band 6	0.″043 × 0.″035	<4.0	~0.022
TCha	Band 3	0.″296 × 0.″170	<18.7	~0.15

Notes. Columns show the target name, the band which flux has been used for the mass estimate, and the estimated inner disk dust mass in Earth mass. The dust masses here reported are highly uncertain. See the text for a more complete discussion.

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