The γ Dor-type pulsations are thought to be driven by a convective blocking mechanism within a convective envelope in a sufficient depth. However, there are several hot γ Dor and hybrid star candidates in which there should not be an adequate convective envelope to excite the γ Dor-type oscillations. In this study we presented the result of examinong these hot variables by spectroscopic and photometric analyses....
The existence of hot γ Doradus and A-F-type hybrid stars
Catanzaro, G.;
2020-01-01
Abstract
The γ Dor-type pulsations are thought to be driven by a convective blocking mechanism within a convective envelope in a sufficient depth. However, there are several hot γ Dor and hybrid star candidates in which there should not be an adequate convective envelope to excite the γ Dor-type oscillations. In this study we presented the result of examinong these hot variables by spectroscopic and photometric analyses....File in questo prodotto:
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