Open AccessCCD u v by β photometry of the young open cluster NGC 663
Author(s) -
Fabregat J.,
Capilla G.
Publication year - 2005
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2005.08712.x
Subject(s) - physics , photometry (optics) , open cluster , distance modulus , astrophysics , stars , cluster (spacecraft) , astronomy , globular cluster , variable star , computer science , programming language
NGC 663 is a young, moderately rich open cluster, known to contain one of the largest fractions of Be stars among all galactic clusters. In this work we present CCD u v by β photometry for stars in its central area. We have used these data to obtain the main cluster physical parameters. We find that the reddening is highly variable, with values ranging from E ( b − y ) = 0.639 ± 0.032 in the central part to E ( b − y ) = 0.555 ± 0.038 in the south‐east. The distance modulus is found to be 11.6 ± 0.1 mag (2.1 kpc) and the age log t = 7.4 ± 0.1 yr (25 +7 −5 Myr) . The age obtained is consistent with the interpretation of the Be phenomenon as an evolutionary effect.