|
par1 | Index1: emissivity index for the inner disk |
par2 | Index2: emissivity index for the outer disk |
par3 | Rbr: break radius separating the inner and outer portions of the disk (gravitational radii) |
par4 | a: dimensionless black hole spin |
par5 | Incl: disk inclination angle to the line of sight (degrees) |
par6 | Rin: inner radius of the disk in units of the radius of marginal stability |
par7 | Rout: outer radius of the disk in units of the radius of marginal stability |
par8 | limb: limb-darkening/-brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) |
norm | flux in line (photons/cm/s) |
The parameters for relconvlp are :
par1 | h: height of the primary source (GM/c2̂) |
par2 | a: dimensionless black hole spin |
par3 | Incl: disk inclination angle to the line of sight (degrees) |
par4 | Rin: inner radius of the disk in units of the radius of marginal stability |
par5 | Rout: outer radius of the disk in units of the radius of marginal stability |
par6 | limb: limb-darkening/-brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) |
par7 | gamma: power-law index of the primary source (E-̂gamma) |
norm | flux in line (photons/cm/s) |
and the parameters for relconvlpext are :
par1 | a: dimensionless black hole spin |
par2 | Incl: disk inclination angle to the line of sight (degrees) |
par3 | Rin: inner radius of the disk in units of the radius of marginal stability |
par4 | Rout: outer radius of the disk in units of the radius of marginal stability |
par5 | limb: limb-darkening/-brightening law with 0=isotropic, 1=darkening (flux 1+2.06mu), 2=brightening (flux ln(1+1/mu)) where mu=cos(emission angle) |
par6 | gamma: power-law index of the primary source (E-̂gamma) |
par7 | hbase: lower height of radially extended primary source |
par8 | htop: upper height of radially extended primary source |
par9 | vbase: velocity of the source at hbase |
par10 | v100: velocity of the source at 100 rg above hbase |
norm | flux in line (photons/cm/s) |
HEASARC Home | Observatories | Archive | Calibration | Software | Tools | Students/Teachers/Public
Last modified: Friday, 23-Aug-2024 13:20:40 EDT
The Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center (GSFC) seeks a creative, innovative individual with strong teamwork and leadership skills to serve as Director of the High Energy Astrophysics Science Archive Research Center (HEASARC). This will be a permanent civil servant position. + Learn more.