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ABSTRACT  Establishing relations between global stellar parameters and asteroseismic quantities can help improve our understanding of stellar astrophysics and facilitate the interpretation of observations. We present an observed relation between the large frequency separation,  Δν , and the frequency of maximum power,  ν max  . We find that  Δν∝ν 0.77  max  , allowing prediction of  Δν  to about 15 per cent given  ν max  . Our result is further supported by established scaling relations for  Δν  and  ν max   and by extended stellar model calculations, which confirm that  Δν  can be estimated using this relation for basically any star showing solar‐like oscillations in the investigated range  (0.5 &lt;  M /M  ⊙  &lt; 4.0) .

The relation between Δν and ν max for solar‐like oscillations