Dear Colleagues, Hitoshi YAMAOKA wrote: > > It is quite likely that a USNO-A2.0 star (position end figures > 07s.150, 37".42, rmag = 17.3, bmag = 17.4) is a quiesient counterpart > of V589 Her. Note that DSS2 R image shows a dim (rmag \sim 19.0) star I find interesting that my astrometry puts the source closer to the proposed counterpart, as my measures are USNO A2.0-based. Regards, Gianluca -- *********************************************************************** * Gianluca Masi "Two things fill the soul * * Via Madonna de Loco, 47 with awe and reverence [...]: * * 03023 Ceccano (FR) the starry sky above me and * * ITALY the moral law within me" * * e-mail: gianmasi@fr.flashnet.it * * web: http://vsnet.eurolink.it/comets/ I. Kant * * Minor Planet Center Obs. Code: 470 - Ceccano * * Center for Backyard Astrophysics - Italy * * VSNET Collaboration Team member * * CCD-astrometry-photometry@egroup mailing-list moderator * ***********************************************************************