Title of article
The Magellanic Stream, High-Velocity Clouds, and the Sculptor Group
Author/Authors
Freeman، Kenneth C. نويسنده , , Putman، Mary E. نويسنده , , Staveley-Smith، Lister نويسنده , , Gibson، Brad K. نويسنده , , Barnes، David G. نويسنده ,
Issue Information
روزنامه با شماره پیاپی 1 سال 2003
Pages
-16
From page
17
To page
0
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
galaxies , Local Group , Interactions , Halo , intergalactic medium , Magellanic Clouds , general , radio lines
Journal title
Astrophysical Journal
Serial Year
2003
Journal title
Astrophysical Journal
Record number
74190
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