Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-05-12
Class.Quant.Grav. 15 (1998) 3131-3145
Astronomy and Astrophysics
Astrophysics
Latex file, 27pages including 10 figures
Scientific paper
10.1088/0264-9381/15/10/016
We consider here the structure of rotating compact objects endowed with a magnetic field in general relativity as models of pulsars. We discuss first the structure of rotating stars in the framework of Hartle taking different realistic equations of state and study their effects on bulk properties of the star. We consider the possibilty of rotating stars with a quark matter core. We further analyse the structure of the magnetic field in the interior of the star as affected by different equations of state as well as due to rotation.
Gupta Anshu
Mishra Amruta
Mishra Hiranmaya
Prasanna A. R.
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