We discuss the nature of eleven Possible Open Cluster Remnants (POCRs) by using absolute proper motions from the
Southern Proper Motion (SPM) Program 3 (Girard et al. 2004) combined with near infrared photometry from 2MASS.
The analysis is done by considering the distribution of stars in the Color-Magnitude and the Vector Point diagrams.
We successfully probed the capabilities of the SPM catalog to detect a physical group by looking at the open cluster
Blanco 1. However, within the uncertainties of the SPM3 catalog and basing on 2MASS photometry we conclude that only
one -ESO282SC26- out of eleven objects turns out to be a probable physical group. We suggest it is an open cluster
1.3 Gyr old and located 1.4 kpc from the Sun.