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Gyoto
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I_nu(nu, T) = cst_*2*h*nu^3/c^2/(exp(h*nu/k*T)-1.);. More...
#include "GyotoSpectrum.h"Go to the source code of this file.
Classes | |
| class | Gyoto::Spectrum::BlackBody |
| Black Body. More... | |
Namespaces | |
| namespace | Gyoto |
| Namespace for the Gyoto library. | |
| namespace | Gyoto::Spectrum |
| Spectrum of a simple object (e.g. a Gyoto::Astrobj::Star) | |
I_nu(nu, T) = cst_*2*h*nu^3/c^2/(exp(h*nu/k*T)-1.);.
h = 6.62606896e-34 J.s; J.s = kg.m^2/s
k = 1.3806504e-23 J.K-1; h/k : s*K = K/Hz.