Unpublished uvby-{beta} photoelectric photometry of the open cluster NGC 6882/5 is presented. Utilizing already tested distance determinations through photometric techniques, it is found that there are at least two distinct star accumulations in the direction of the open cluster NGC 6882/5. A brief discussion is made of the nature of the previously found short period variables.
Cone search capability for table J/other/RMxAA/44.111/table3 ({beta} photoelectric photometry of the stars in the direction of NGC 6882)