ROTATING COMPACT OBJECTS WITH MAGNETIC-FIELDS

We consider here the structure of rotating compact objects endowed wit h a magnetic field in general relativity as models of pulsars. We disc uss the structure of rotating stars in the framework of Hartle, taking different realistic equations of state, and study their effects on bu lk properties of stars. We consider the possibility of rotating stars with a quark matter core. We also analyse the structure of the magneti c field in the interior of the star, as affected by different equation s of state, as well as due to rotation.