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[vsnet-rcb 86] Re: vsnet-rcb 85



> If these stars are of normal A-star
> like objects, then what would be the cause of 'fading' resembling those
> of RCB stars?  

The light fading of these stars are distinguishing from those of the RCB: 
"fast" decline during days (hot star, V348 Sgr) or tens of days (cold stars) 
and then the slower recovering of normal light. i.e. a light curve has the 
very typical shape. An unvisibelity of star, as this was in the case of LO Cep, 
and CT Vul, etc, does not mean it is a star with the RCB variability.    
First condition is a full light curve. 

Alexander 

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