Statistics – Computation
Scientific paper
Apr 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976c%26t....92...65d&link_type=abstract
Ciel et Terre, vol. 92, Mar.-Apr. 1976, p. 65-104. In French.
Statistics
Computation
Astrometry, Binary Stars, Celestial Mechanics, Dynamic Characteristics, Orbit Calculation, Parallax, Stellar Motions, Computer Techniques, Mathematical Models, Stellar Luminosity, Stellar Mass, Tables (Data)
Scientific paper
A general survey on the various kinds of dynamical parallaxes is given, as well as an intercomparison of the methods used today for the computation of the orbital and nonorbital ones. The methods of Russell-Moore and of Baize-Romani are especially discussed and compared in the case of orbital parallaxes. Between the three methods known for computing the nonorbital parallaxes, the method of Russell is shown to be the most efficient one. The terminology is discussed and proposals are made. Nonlinearity of the mass-luminosity relation does not complicate the present mathematical process used for computing dynamical parallaxes, orbital or non-orbital ones.
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