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Table 4

Membership of the programme objects.

Cluster CP Star Membership
μ/ν/ph/π final

Cr 132 HD 56343 y/−/y/n − (p)a
IC 4725 BD−19 5044L p/−/p/− p (p)
HD 170836 y/y/p/− y (p)
HD 170860 p/nb/y/− p (p)
NGC 2516 CP−60 944 y/−/y/− y (y)a
HD 65712 y/−/y/− p (y)a
HD 66295 y/y/y/− y (y)
NGC 3114 HD 87240 p/y/y/− p (n)a
HD 87405 p/n/y/p ? (?)a
HD 87752 p/y/y/− y (−)
HD 304841 p/−/y/− p (p)
HD 304842 p/y/y/− y (p)
NGC 3228 HD 89856 p/−/n/p n (n)a
HD 298053 p/−/y/− p (p)
NGC 3532 HD 96040 p/−/p/− p (p)
HD 96729 p/−/n/− n (?)a
NGC 5460 HD 122983 y/−/p/− p (p)
HD 123225 y/−/y/− y (y)
NGC 5662 CP−56 6330 n/−/y/− n (n)a
HD 127924 y/−/p/p p (y)
NGC 6281 HD 153947 p/−/n/− n (−)a
HD 153948 y/p/y/− y (y)
NGC 6405 CD−32 13119 p/−/y/− p (p)
HD 318100 y/y/y/− y (y)
HD 318107 y/−/y/− y (y)
NGC 6475 HD 162305 y/y/y/− y (y)
HD 320764 y/y/y/− y (p)

Notes. The final membership was deduced from individual ones based on proper motion (μ), radial velocity (ν), position in the HRD (ph), and parallaxes (π). In parenthesis, the membership obtained by Landstreet et al. (2007) is given.

(a)

membership discussed in the text;

(b)

only a single measurement by Landstreet et al. (2008); binarity cannot be excluded.

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