Fr. Ferraro et al., BINARY STARS IN GLOBULAR-CLUSTERS - DETECTION OF A BINARY SEQUENCE INNGC-2808, Astronomy and astrophysics, 327(2), 1997, pp. 598-601
A CCD V,V - I colour-magnitude diagram (CMD) of the Galactic globular
cluster NGC 2808 has been obtained with the ESO-NTT, reaching down to
V similar to 24.The highly populated Main Sequence (MS) presents a sig
nificant broadening redward to the MS ridge line, larger than expected
from photometric errors alone, which could be interpreted as due to b
inary candidates.