Up: Nice observatory measurements of series)
In previous papers (Thorel 1996, 1998, 2000)
we presented measurements of
double stars made at Nice with the 50 cm equatorial refractor equipped with a
wire micrometer and an electronic recording device. The research program
proposed by Dommanget is aimed at completing the CCDM catalogue
(resolution of ambiguities in the binarity characteristics and the position
of certain double stars which have seldom or never been observed again since
the epoch or their discovery; cf. Dommanget & Nys 1999).
Up: Nice observatory measurements of series)
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