RT @kirxkirx: @TM_Eubanks @IlanYLevine The slope is close to that of the Rayleigh–Jeans law. This might be thermal emission from an optical…
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@TM_Eubanks @IlanYLevine The slope is close to that of the Rayleigh–Jeans law. This might be thermal emission from an optically thick source that is slightly non-uniform (so the slope is not exactly 2.0). Here is the relevant plot from https://t.co/TO4Khm2
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Ghisellini, G: Radiative Processes in High Energy Astrophysics[...] http://t.co/Kyy6sedi8c #adsarticleoftheday
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Radiative Processes in High Energy Astrophysics http://t.co/YZQ61vki