Title of article :
The Quiescent Counterpart of the Soft Gamma-Ray Repeater SGR 0526-66
Author/Authors :
Murakami، T. نويسنده , , Kaplan، D. L. نويسنده , , Kulkarni، S. R. نويسنده , , Frail، D. A. نويسنده , , Marshall، H. L. نويسنده , , Yonetoku، D. نويسنده ,
Issue Information :
روزنامه با شماره پیاپی 2 سال 2003
Abstract :
We assemble the equations of general relativistic magnetohydrodynamics (MHD) in 3 + 1 form. These consist of the complete coupled set of Maxwellʹs equations for the electromagnetic field, Einsteinʹs equations for the gravitational field, and the equations of relativistic MHD for a perfectly conducting ideal gas. The adopted form of the equations is suitable for evolving numerically a relativistic MHD fluid in a dynamical spacetime characterized by a strong gravitational field.
Keywords :
neutron , X-rays , SGR 0526-66 , Individual , Pulsars , stars
Journal title :
Astrophysical Journal
Journal title :
Astrophysical Journal
