Title of article
A Far Ultraviolet Spectroscopic Explorer Survey of Molecular Hydrogen in Intermediate-Velocity Clouds in the Milky Way Halo
Author/Authors
Savage، Blair D. نويسنده , , Sembach، Kenneth R. نويسنده , , Richter، Philipp نويسنده , , Wakker، Bart P. نويسنده ,
Issue Information
روزنامه با شماره پیاپی 1 سال 2003
Pages
-22
From page
23
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
Galaxy , ISM , Abundances , clouds , quasars , absorption lines , Ultraviolet , Halo
Journal title
Astrophysical Journal
Serial Year
2003
Journal title
Astrophysical Journal
Record number
74200
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