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[vsnet-newvar 558] re HadV67 ID




> New Haseda variable (HadV67)
>
> Katsumi Haseda (Aichi, Japan) reports the discovery of a new variable
> star (HadV67). The identity with V648 Oph needs to be checked.

There is nothing at V648 Oph's catalogue position on survey plates.

V648 Oph lies roughly due West of HadV67 by about 50 years of precession
worth of RA.

Brighter magnitudes quoted for HadV67 fit the value for maximum of V648 Oph
pretty well.

IMPORTANT : The GCVS period for V648 Oph is 169 days, the dates quoted for
brightest light of HadV67 in vsnet-newvar 557 are quite consistent with
this period.

Only reference I can find is SCHNELLER*GUL*2.5.2 (1961), but note that the
GCVS quoted epoch is in 1929.

John



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