Publications of the Astronomical Society of the Pacific, Vol. 117, No. 833 (July 2005), pp. 711-720 (10 pages) ABSTRACT The shape of the line bisector for the prototype spectral line Fe i λ6253 was ...
Van Vleck and Weisskopf 1, in an interesting paper, have shown that the well-known Lorentz formula for the shape of a spectral line is incorrect except at frequencies close to the resonance frequency.
Black hole spin, or angular momentum, is a fundamental property determined by the rotation of the black hole's event horizon, influenced by the progenitor star's rotation and conserved during collapse ...
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