palPrebn palPrebn - Generate the matrix of precession between two objects (old)

Description:

Generate the matrix of precession between two epochs, using the old, pre-IAU1976, Bessel-Newcomb model, using Kinoshita's formulation

Invocation:

void palPrebn ( double bep0, double bep1, double rmatp[3][3] );

Arguments:

bep0 = double (Given)

Beginning Besselian epoch.

bep1 = double (Given)

Ending Besselian epoch

rmatp = double[3][3] (Returned)

precession matrix in the sense V(BEP1) = RMATP $*$ V(BEP0)

See Also

Kinoshita, H. (1975) 'Formulas for precession', SAO Special Report No. 364, Smithsonian Institution Astrophysical Observatory, Cambridge, Massachusetts.