compLS: Comptonization, Lamb & Sanford

A Comptonization spectrum after Lamb & Sanford (1979, MNRAS 288, 555). This model calculates the self-Comptonization of a bremsstrahlung emission from an optically thick spherical plasma cloud with a given optical depth and temperature. It was popular for Sco X-1.

par1	temperature in keV
par2	optical depth
norm	normalization #50076#>

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Last modified: Tuesday, 28-May-2024 10:09:22 EDT