Gyoto
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A geometrically thin, optically thick disk. More...
#include <iostream>
#include <fstream>
#include <iomanip>
#include <GyotoThinDisk.h>
#include <GyotoBlackBodySpectrum.h>
Go to the source code of this file.
Classes | |
class | Gyoto::Astrobj::PageThorneDisk |
Geometrically thin disk in Kerr metric. More... | |
Namespaces | |
Gyoto | |
Namespace for the Gyoto library. | |
Gyoto::Astrobj | |
Access to astronomical objects. | |
A geometrically thin, optically thick disk.
This class describes a disk contained in the z=0 (equatorial) plane, extending from r=r_ISCO to r=infinity. The flux emitted at radius r is given by Page & Thorne (1974, ApJ 191:499, Eqs. 11b, 14, 15).
Only bolometric flux is implemented (as quantity User4), no spectral resolution.