This resulted in Fig. 1. Unfortunately the astrometry of BD +69◦1231 is itself somewhat problematic due to the surrounding bright nebulosity and the location of the CVF image on the op- tical image is correspondingly uncertain.
This resulted inFig. 1. Unfortunately the astrometry of BD +69◦1231 isitself somewhat problematic due to the surrounding brightnebulosity and the location of the CVF image on the op-tical image is correspondingly uncertain.