Impact of discontinuous grain size distributions on the spectral energy distribution of debris disks

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Table 2

Stellar, disk, and dust model parameters for the simulations and their reference.

SpT (exemplary system)	Temperature	Radius	Narrow belt	Broad belt	Blow-out grain size
	(K)	(R_⊙)	R_in, R_out (au)	R_in^,R_out (au)	a_bo (µm)
A star (β Pictoris)	8052 ^(a)	1.8 ^(b)	92, 109	37, 163	1.99
F star (HD 139664)	6681 ^(c)	1.26 ^(d)	76, 90	31, 136	1.05
G star (HD 107 146)	5820 ^(e)	0.993 ^(e)	62, 73	25, 110	0.43
K star (HD 53 143)	5224 ^(f)	0.85 ^(g)	57, 67	23, 101	–
M star (AU mic)	3500 ^(h)	0.5 ^(h)	38, 45	15, 68	–

Notes. The chosen stellar parameters were selected as one of the representative stars for each spectral type.

References. ^(a)Gray et al. (2006). ^(b)Kervella et al. (2004). ^(c)Reiners (2006). ^(d)Rhee et al. (2007). ^(e)Marino et al. (2018). ^(f)Kalas et al. (2006). ^(g)Watson et al. (2011). ^(h)Donati et al. (2023).

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