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Astron. Astrophys. 335, 679-684 (1998)

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Appendix

The normalized components [FORMULA] of the (symmetric) correlation tensor [FORMULA] are

[EQUATION]

They have to be inserted into Eqs. (30) and (34) yielding the inhomogeneous equation system which is solved with the boundary conditions (35).

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© European Southern Observatory (ESO) 1998

Online publication: June 18, 1998
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