Star Clustering Near the NGC 68-72 Group of Galaxies

Abstract

A study of star clustering near the NGC 68-72 group of galaxies indicates the clustering is apparently only a fluctuation in foreground star density.

Leave a Comment

Fill in your details below or click an icon to log in:

WordPress.com Logo

You are commenting using your WordPress.com account. Log Out /  Change )

Facebook photo

You are commenting using your Facebook account. Log Out /  Change )

Connecting to %s