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Where is the reference to Eddington's original paper? 129.21.81.116 ( talk) 16:30, 17 April 2012 (UTC)
The following assertion is dubious, and I have removed it:
The spherical approximation is commonly used, but it is always understood to be an approximation only. When the actual geometry of accretion discs is taken into account, it is found that the results can differ considerably from the classical value. See Heinzeller and Duschl(2006). Stigmatella aurantiaca ( talk) 10:34, 11 December 2013 (UTC)
This article Brightest neutron star yet has a multipolar magnetic field gives another possible mechanism for superluminosity. — Preceding unsigned comment added by Jetpen ( talk • contribs) 02:01, 25 February 2017 (UTC)
This
level-5 vital article is rated Start-class on Wikipedia's
content assessment scale. It is of interest to the following WikiProjects: | |||||||||||
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Where is the reference to Eddington's original paper? 129.21.81.116 ( talk) 16:30, 17 April 2012 (UTC)
The following assertion is dubious, and I have removed it:
The spherical approximation is commonly used, but it is always understood to be an approximation only. When the actual geometry of accretion discs is taken into account, it is found that the results can differ considerably from the classical value. See Heinzeller and Duschl(2006). Stigmatella aurantiaca ( talk) 10:34, 11 December 2013 (UTC)
This article Brightest neutron star yet has a multipolar magnetic field gives another possible mechanism for superluminosity. — Preceding unsigned comment added by Jetpen ( talk • contribs) 02:01, 25 February 2017 (UTC)