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[vsnet-chat 6278] V1860 Sgr oscillations



   According to the ASAS-3 data, V1860 Sgr (previously reported
to be RCB: star, presently not considered to belong to this
type) shows relatively regular variations (amplitude 0.3 mag)
with a period of 40-50 d.  This periodicity is characteristic
to R CrB-type variations at maximum.  Although spectroscopic
observation is against the classification as an R CrB star, this
star probably needs more detailed examination.

Regards,
Taichi Kato


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