Solar-like oscillations in the G9.5 subgiant β Aquilae

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Table 2

Asymptotic parameters as derived by a linear weighted least-squares fit to the asymptotic relation (4).

Δν (μHz)	δν₀₂ (μHz)	ϵ

29.56 ± 0.10	2.55 ± 0.71^a	1.29 ± 0.04

Notes.

^(a)

The most likely value for the small separation was derived by using the definition from the asymptotic relation with the couples of frequencies (ν_12,0,ν_11,2), (ν_13,0,ν_12,2) and (ν_16,0,ν_16,2 − Δν).

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