|
par1 | eta, ratio of the disk power produced by a torque at the disk
inner boundary to the disk power arising from accretion. It must be
![]() ![]() |
par2 | specific angular momentum of the black hole in units of the
black hole mass M (geometrized units G=c=1). Should be ![]() |
par3 | disk's inclination angle (the angle between the axis of the
disk and the line of sight). It is expressed in degrees. i=0 is for a
"face-on" accretion disk. i should be ![]() |
par4 | the mass of the black hole in units of the solar mass. |
par5 | the “effective” mass accretion rate of the disk in units of
![]() ![]() |
par6 | the distance from the observer to the black hole in units of kpc. |
par7 | spectral hardening factor, T![]() ![]() |
par8 | a flag to switch on/off the effect of self-irradiation (never
allowed to be free). Self-irradiation is included when >
0. Self-irradiation is not included when ![]() |
par9 | a flag to switch on/off the effect of limb-darkening (never
allowed to be free). The disk emission is assumed to be limb-darkened
when >0. The disk emission is assumed to be isotropic when
lflag is ![]() |
K | normalization. Should be set to 1 if the inclination, mass and distance are frozen. |
Parameters for zkerrbb:
par1 | eta, ratio of the disk power produced by a torque at the disk
inner boundary to the disk power arising from accretion. It must be
![]() ![]() |
par2 | specific angular momentum of the black hole in units of the
black hole mass M (geometrized units G=c=1). Should be ![]() |
par3 | disk's inclination angle (the angle between the axis of the
disk and the line of sight). It is expressed in degrees. i=0 is for a
"face-on" accretion disk. i should be ![]() |
par4 | the mass of the black hole in units of the solar mass. |
par5 | the “effective” mass accretion rate of the disk in units of
![]() ![]() |
par6 | the redshift of the black hole. |
par7 | spectral hardening factor, T![]() ![]() |
par8 | a flag to switch on/off the effect of self-irradiation (never
allowed to be free). Self-irradiation is included when >
0. Self-irradiation is not included when ![]() |
par9 | a flag to switch on/off the effect of limb-darkening (never
allowed to be free). The disk emission is assumed to be limb-darkened
when >0. The disk emission is assumed to be isotropic when
lflag is ![]() |
K | normalization. Should be set to 1 if the inclination, mass and distance are frozen. |
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Last modified: Tuesday, 28-May-2024 10:09:22 EDT