Introduction A non-perturbative general relativistic approach to global astrometry was developed by de Felice et al. (1998) to handle satellite astrometry data in a genuine relativistic framework. In ...
The end state of a coalescing binary of compact objects depends strongly on the final total mass M and angular momentum J . Since gravitational radiation emission causes a slow evolution of the binary...
The end state of a coalescing binary of compact objects depends strongly on the final total mass M and angular momentum J . Since gravitational radiation emission causes a slow evolution of the binary...
Introduction 1.1. Considerons (m + 1) fonctions polynomiales # i (x 1 , . . . , xm ) de (m + 1) variables a coe#cients complexes, homogenes de meme degre et non toutes identiquement nulles; on leur as...