Title of article
Chandra Observations of A2029: The Dark Matter Profile Down to below 0.01rvir in an Unusually Relaxed Cluster
Author/Authors
Buote، David A. نويسنده , , Lewis، Aaron D. نويسنده , , Stocke، John T. نويسنده ,
Issue Information
روزنامه با شماره پیاپی 1 سال 2003
Pages
-134
From page
135
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
individual (A2029) , X-rays , intergalactic medium , cosmological parameters , Dark matter , galaxies , Clusters
Journal title
Astrophysical Journal
Serial Year
2003
Journal title
Astrophysical Journal
Record number
74182
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