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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
vsnet-adm@kusastro.kyoto-u.ac.jp
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp