Abstract
Le flux (2-10 keV) a augmente de 1,6×10 −9 a 2,5×10 −9 erg•cm −2 •s −1 au cours des observations (17-18 juillet 1983) et cette augmentation a ete accompagnee d'une croissance de l'indice de 1,7 a 2,1 et d'une diminution de la coupure aux hautes energies. Le spectre en loi de puissance est compatible avec un modele dans lequel des photons mous emis de la surface de l'etoile a neutron sont comptonises dans un plasma chaud entourant l'etoile
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