The oEA Stars

Physics

Scientific paper

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Scientific paper

We present the revised list of presently known oscillating mass-accreting components of semi-detached Algol-type eclipsing binaries (oEA stars) and discuss the pulsation mode visibility and strategies of mode identification. On the example of the best studied oEA star RZ Cas we discuss the reasons for the observed orbital modulation of the pulsation amplitude.

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