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We carried out a multicolour time‐series photometric study of six stars claimed as ‘hybrid’ p and g mode pulsators in the literature. γ Peg was confirmed to show short‐period oscillations of the β Cep type and simultaneous long‐period pulsations typical of Slowly Pulsating B (SPB) stars. From the measured amplitude ratios in the Strömgren  uvy  passbands, the stronger of the two short period pulsation modes was identified as radial; the second is  ℓ= 1 . Three of the four SPB‐type modes are most likely  ℓ= 1  or 2. Comparison with theoretical model calculations suggests that γ Peg is either a  ∼8.5 M ⊙   radial fundamental mode pulsator or a  ∼9.6 M ⊙   first radial overtone pulsator. HD 8801 was corroborated as a ‘hybrid’δ Sct/γ Dor star; four pulsation modes of the γ Dor type were detected, and two modes of the δ Sct type were confirmed. Two pulsational signals between the frequency domains of these two known classes of variables were confirmed and another was newly detected. These are either previously unknown types of pulsation or do not originate from HD 8801. The O‐type star HD 13745 showed small‐amplitude slow variability on a time‐scale of 3.2 d. This object may be related to the suspected new type of supergiant SPB stars, but a rotational origin of its light variations cannot be ruled out at this point. 53 Psc is an SPB star for which two pulsation frequencies were determined and identified with low spherical degree. Small‐amplitude variability was formally detected for 53 Ari but is suspected not to be intrinsic. The behaviour of ι Her is consistent with non‐variability during our observations, and we could not confirm light variations of the comparison star 34 Psc previously suspected. The use of signal‐to‐noise criteria in the analysis of data sets with strong aliasing is critically discussed.

monthly notices of the royal astronomical society

Confirmation of simultaneous p and g mode excitation in HD 8801 and γ Peg from time‐resolved multicolour photometry of six candidate ‘hybrid’ pulsators