Abstract
As a part of an ungoing observational program to determine astrometric positions for objects associated with molecular clouds and/or located in regions of recent star formation, we report in this work results for Herbig emission-line objects in the regions of NGC 7000 and IC 5070. Herbig's original positions are 10 aresec of the astrometrically determined positions. In particular, the astrometric position for V1057 Cyg agrees within 1 arcsec with the position of OH maser in the region, confirming the physical association between the two objects.
