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The δ Scuti Pulsator Occurrence as a Function of Age, Teff, Rotation, and Metallicity

  • Authors: Ian Berry, Daniel Huber, Yaguang Li, Daniel Hey, Timothy R. Bedding, Simon J. Murphy

Ian Berry et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Stacked amplitude spectrum of all δ Scuti pulsators in this study. Clusters are ordered by age (youngest on top). The red dotted lines separate each cluster. Within each cluster, stars are sorted by Teff, with the coolest on top. Note the appearance of δ Scuti stars with regular pulsation patterns in the younger (≲200 Myr) open clusters.

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