Dust::MMPUV Class Reference
The radiation field published by Mezger, Mathis and Panagia. More...
#include <mmpradfield.hxx>
Inheritance diagram for Dust::MMPUV:
Collaboration diagram for Dust::MMPUV:
Public Member Functions | |
| MMPUV (double chi) | |
| These are the methods for the MMPUV class. | |
| virtual double | operator() (double E) |
Detailed Description
The radiation field published by Mezger, Mathis and Panagia.Constructor & Destructor Documentation
| Dust::MMPUV::MMPUV | ( | double | chi | ) |
These are the methods for the MMPUV class.
Returns the radiation field of Mezger, Mathis and Panagia ( 1982A&A...105..372M ) as ammended in the 1983 paper. chi controls the scaling of the field.
Member Function Documentation
| double Dust::MMPUV::operator() | ( | double | E | ) | [virtual] |
The Specific Energy density. E must be specified in the units of Joules (using SI throughout). More precisely this is energy per unit volume per unit energy interval. At some time I convinced my self that this is equivalent to the (number of photons) m^-3, but not sure any more. Anyway, u_E dE than has the units of J m^-3. Conversion to flux can be done using the speed of light. (inerited from UnaryDD)
Implements Dust::RadField.
The documentation for this class was generated from the following files:
