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 | |
namespace | Gyoto |
Namespace for the Gyoto library. | |
namespace | 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.