arXiv:astro-ph/0512553AbstractReferencesReviewsResources
Comments on "Perspectives on Galactic Dynamics via General Relativity"
Published 2005-12-22Version 1
In this comment we question some arguments presented in astro-ph/0512048 to refuse the presence of an singular mass surface layer. In particular, incorrect expressions are used for the disk's surface mass density. We also point out that the procedure of removing the descontinuity on the $z=0$ plane with a region of continuous density gradient generates other two regions of descontinuities with singular mass surface layers making the model unrealistic.
Comments: 5 pages, 1 figure
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arXiv:astro-ph/0610370 (Published 2006-10-12)
Galactic Dynamics via General Relativity: A Compilation and New Developments
arXiv:astro-ph/0512048 (Published 2005-12-02)
Perspectives on Galactic Dynamics via General Relativity
Rotating Collapse of Stellar Iron Cores in General Relativity