Abstract:We have presented BVR surface photometry and geometric analyses for galaxy pair KPG 578 a, b (NGC 7537, NGC 7541). The contour maps, BVR surface brightness profiles (SB) and geometric profiles (x c , y c , PA and Ellip = 1 − b/a) have been used for each galaxy in the pair. The galaxy pair KPG 578 is an intermediate pair with projected separation = − r 35.4 h kpc p 70 1 and relative velocity = v Δ 15 km/s. The total orbital mass of KPG 578 is determined to be = ⊙ M x M 6. 03 10 t 9
Set email alert for when this publication receives citations?
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.