Balona, L. A; Engelbrecht, C. A; Joshi, Y. C; Joshi, S; Sharma, K; Semenko, E; Pandey, G; Chakradhari, N. K; Mkrtichian, D; Hema, B. P; Nemec, J. M
(Oxford University Press on behalf of the Royal Astronomical Society, 2016-09)
The hot
γ
Doradus stars have multiple low frequencies characteristic of
γ
Dor or SPB variables,
but are located between the red edge of the SPB and the blue edge of the
γ
Dor instability
strips where all low-frequency ...