Individual sheet: CC Cas
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Spectral type(s): O8.5III + B0V
Multiplicity:
Confirmed binary system
Period(s): ~3 d
Orbital solution: no
Ref:
Comments:
The radio variations (Gibson & Hjellming 1974) might be attributed to eclipse-like variations (variation of the free-free absorption as a function of the orbital phase), and not necessarily to a non-thermal origin.