1997/07/12 by F. R. Ferraro, Ferraro, F. R., E. Carretta +5
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9707139
4 pages, Latex, uses l-aa.sty, plus 3 .ps figures, accepted by Astronomy and Astrophysics, also available at http://www.bo.astro.it/bap/BAPhome.html as bap97-20-*.ps or via anonymous ftp at ftp://boas3.bo.astro.it/bap/files/ as bap97-20-*.ps
arxiv created 1997/07/12 · arxiv updated 2009/12/01
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 ~ 24. The highly populated Main Sequence (MS) presents a significant broadening redward to the MS ridge line, larger than expected from photometric errors alone, which could be interpreted as due to binary candidates.