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[vsnet-campaign 701] V344 Ori: the position and the quiscent counterpart
Dear all,
> The quiescent counterpart has been suggested to be a 18-th mag USNO
> star, which is not markedly blue. This may suggest that the true
> quiescence of V344 Ori may be fainter. (see, however, the
> spectroscopic observation given in Munari et al. A&AS 122, 495,
> which shows strong balmer emission lines).
I have done astrometry of V344 Ori with the Kyoto image taken on
Jan. 16 with 25 GSC-ACT stars as: R.A. = 6h15m18s.92, Decl. =
+15o30'59".7. The accuracy is better than 0".5, perhaps 0".3 level.
It agrees very well with DWS97 position (end figures 18s.9, 31'00")
The suggestion that the USNO_A2.0 star (position end figures
18s.962, 59".98, r=17.8, b=18.4) is a quiscent counterpart is very
plausible.
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
vsnet-adm@kusastro.kyoto-u.ac.jp
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