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Gyoto
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A thick accretion disk described by its opening angle between the BH spin axis and the disk surface, and its inner radius. More...
#include <iostream>#include <fstream>#include <iomanip>#include <GyotoStandardAstrobj.h>#include <GyotoKappaDistributionSynchrotronSpectrum.h>#include <GyotoThermalSynchrotronSpectrum.h>Go to the source code of this file.
Classes | |
| class | Gyoto::Astrobj::ThickDisk |
| A thick accretion disk described by its opening angle between the BH spin axis and the disk surface, and its inner radius. More... | |
Namespaces | |
| Gyoto | |
| Namespace for the Gyoto library. | |
| Gyoto::Astrobj | |
| Access to astronomical objects. | |
A thick accretion disk described by its opening angle between the BH spin axis and the disk surface, and its inner radius.
Density is assumed to follow a r^{-2} law while temperature is a power law with a specified slope.
This astrobj emits thermal synchrotron.
1.8.17