Physics
Scientific paper
Mar 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009coast.159...42h&link_type=abstract
"Communications in Asteroseismology, Vol. 159, p. 42-44. Proceedings of "JENAM 2008 Symposium No 4: Asteroseismology and Stellar
Physics
4
Scientific paper
We carried out a multi-colour time-series photometric study of six stars that were claimed as ''hybrid'' p- and g-mode pulsators in the literature. The β Cep/SPB star γ Peg was confirmed and revealed excellent asteroseismic potential. HD 8801 was confirmed as a ''hybrid'' δ Sct/γ Dor star; additional pulsation frequencies were detected. 53 Psc likely is an SPB star and the O-type star HD 13745 showed small-amplitude slow variability. No light variations were detected for HD 19374 and, surprisingly, ι Her.
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