δ Scuti and γ Doradus stars

Details δ Scuti and γ Doradus stars δ Scuti and γ Doradus stars

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..224..335b&link_type=abstract

The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss,

Physics

1

Stars: Variables: Δ Scuti, Stars: Oscillations (Including Pulsations).

Scientific paper

The paper emphasizes the connection between observations and theory in
the Lower Instability Strip. It is argued that the δ Scuti and
γ Doradus pulsators are very close relatives in the sense that the
γ Doradus phenomenon can also be seen in the slightly hotter
δ Scuti variables.

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