Observational evidence for a possible link between PAH emission and dust trap locations in protoplanetary disks

Open Access

Table B.1

Best-fit parameters SEDs

Target	$M_{d i s k}^{a}$ $M_{\rm disk}^a$ (10⁻³ M_⊙)	h_c	r_cav (au)	δ_dust
V892Tau	4	0.05	23	10⁻³
HD100453	2	0.20	32	10⁻²
HD100546	8	0.20	30	10⁻¹
HD139614	6.6	0.10	13	10⁰
SR21	4	0.15	60	10⁻³
SYCha	10	0.10	106	10⁰
TCha	10	0.10	28	10⁻¹

^a) M_disk is the total disk gas mass: the disk dust mass is computed within RADMC-3D assuming a gas-to-dust ratio of 100.

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