The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) - X. Interpreting the peculiar dust rings around HD 131835

Open Access

Table 1

Different $Q_{D, s}^{*}$ $Q_{D, s}^{*}$ and b_s values for the modelled belts.

Identifier	$Q_{D, s}^{} [erg / g]$ $Q_{D, s}^{}[\mathrm{erg} / \mathrm{g}]$	b_s
Basalt	5 · 10⁶	−0.37
Very strong	5 · 10⁸	−0.37
Strong	5 · 10⁷	−0.37
Weak	5 · 10⁵	−0.37
Very weak	5 · 10⁴	−0.37
Extremely weak	5 · 10³	−0.37
Steep slope	5 · 10⁶	−1
Flatter slope	5 · 10⁶	−0.05

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