|
par1 | distance (kpc) |
par2 | spectral hardening factor, Tcol/Teff. Should be greater than 1.0, and considered to be 1.5–1.9 for accretion disks around a stellar-mass black hole. See, e.g., Shimura & Takahara (1995) 445, 780 |
par3 | mass of the central object (solar unit) |
par4 | mass accretion rate ( g/s) |
par5 | disk inclination angle (deg; 0 for face-on) |
par6 | inner radius (units of ). 1.235 is the last stable orbit. |
par7 | outer radius (units of ) |
K | normalization factor. should be fixed to 1. |
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Last modified: Friday, 23-Aug-2024 13:20:40 EDT
HEASARC Staff Scientist Position - Applications are now being accepted for a Staff Scientist with significant experience and interest in the technical aspects of astrophysics research, to work in the High Energy Astrophysics Science Archive Research Center (HEASARC) at NASA Goddard Space Flight Center (GSFC) in Greenbelt, MD. Refer to the AAS Job register for full details.