UBVI CCD photometry of M35 (NGC 2168)

Details UBVI CCD photometry of M35 (NGC 2168) UBVI CCD photometry of M35 (NGC 2168)

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.306..361s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 306, Issue 2, pp. 361-370.

Astronomy and Astrophysics

Astronomy

51

Hertzsprung, Russell (Hr) Diagram, Open Clusters And Associations: Individual: M35 (Ngc 2168)

Scientific paper

UBVI CCD photometry has been obtained for the intermediate-age open cluster M35 (NGC 2168). From this new photometry we derived the cluster parameters (V_0 - M_V= 9.60 +/- 0.10 mag, E(B-V) = 0.255 +/- 0.024 mag), age (log t_age=8.3 +/-0.3) and a photometric abundance (Z ~ 0.008, i.e. [Fe/H] ~ - 0.3) from comparison with theoretical isochrones of the Padova group. A minimum binary frequency (35 +/- 5 per cent) was estimated from the distribution of distance moduli of unevolved proper motion members. Faint photometric members were selected by using differences in the reddening effect on colour indices.

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