NSV 7814: A Probable Eclipsing Binary (Abstract)

Volume 20 number 2 (1991)

Robert DeMartino

West Haven, CT

Christopher Predom

East haddam, CT

Abstract

(Abstract only) NSV 7814 was first observed to vary around the turn of the century when K. Graff (1921, Astron. Nachr., 213, 176) used it as a comparison star for observations of SS Her. Our data span 548 days and total 84 magnitude estimates. The observations suggest a very short period eclipsing binary that varies from visual magnitude 11.2 to 12.2.