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[vsnet-newvar 495] Re: re Haseda Variable 62 ID
- Date: Sat, 8 Jul 2000 22:04:50 +0900 (JST)
- To: vsnet-newvar
- From: Taichi Kato <tkato>
- Subject: [vsnet-newvar 495] Re: re Haseda Variable 62 ID
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
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
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp