Title of article
Keck Spectroscopy and Hubble Space Telescope Imaging of GRB 000926: Probing a Host Galaxy at z = 2.038
Author/Authors
Bloom، J. S. نويسنده , , Kulkarni، S. R. نويسنده , , Galama، T. J. نويسنده , , Castro، S. نويسنده , , Harrison، F. A. نويسنده , , Holtzman، J. A. نويسنده , , Djorgovski، S. G. نويسنده ,
Issue Information
روزنامه با شماره پیاپی 1 سال 2003
Pages
-127
From page
128
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
gamma rays , bursts , high-redshift , galaxies
Journal title
Astrophysical Journal
Serial Year
2003
Journal title
Astrophysical Journal
Record number
74180
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