| Gyoto
    | 
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.
 1.8.14
 1.8.14