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[vsnet-newvar 495] Re: re Haseda Variable 62 ID



Re: [vsnet-newvar 494] re Haseda Variable 62 ID

> pretty significant proper motions are given of RA 151+/-15 mas and Dec
> -68.5+/-19 mas [where mas = milliarcseconds.  UCAC1 mags are in a
> passband that lives between Johnson V and R]

   I simply considered the large proper motion is an apparent one, that
is from identifications of different stars (or combined stellar images)
overlapped on this large-amplitude variable.

   However, if the star is a genuine low-luminosity star with conspicuous
variablity, it may be a discovery of quite unique nature (the significance
may even surpass, dependeing on the nature, Haseda's discovery of Nova Sct
2000).

   I hope the apparent discrepancy would soon be positively solved.  The
object is reported bright now, and provides a great opportunity before
it returns to dormancy again.

Regards,
Taichi Kato

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