Brey 73 - A multiple Wolf-Rayet star
Résumé
CCD images of the WR star Brey 73 were obtained with a 2.2-m telescope in October, 1987. The CAPELLA software package for profile fitting photometry (Debray et al., 1988) was used. The results show that Brey 73 is an aggregate of 11 components. The apparent and absolute magnitudes of the aggregate are determined.