CCD UBV RI photometry of the open cluster Berkeley 8

Abstract

The poorly studied Berkeley 8 (Be 8) open cluster is analyzed from CCD UBV RI photometric data takenwith the 0.90 m telescope at the Sierra Nevada Observatory. The Z = +0.008 PARSEC isochrone gave us a reddeningof E(B-V) = 0.69 ± 0.03, a distance of 3410 ± 300 pc, and an age of 2.8 ± 0.2 Gyr. Its median Gaia DR2 distance,d = 3676 ± 810 pc, is in good agreement with our photometric distances, 3410–3620 pc within the uncertainties. Thekinematic parameters of five likely members of Be 8 with the circular orbits, ecc = [0.23, 0.30] , reflect the propertiesof the Galactic thin disc, which is also consistent with what is expected of its metal content ([M/H] = –0.27). Be 8with R > 9 kpc (co-rotation gap at 9 kpc) may have been originating from a different galactic radius or different starformation region.