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.
cflow: cooling flow
A cooling flow model after Mushotzky & Szymkowiak (Cooling Flows in
Clusters and Galaxies, ed. Fabian, 1988). An index of zero for the
power-law emissivity function corresponds to emission measure weighted by
the inverse of the bolometric luminosity at that temperature. The abundance
ratios are set by the abund command. Redshift is converted to
distance using the cosmology set by the cosmo command.
par1 |
index for power-law emissivity function |
par2 |
low temperature (keV) |
par3 |
high temperature (keV) |
par4 |
abundance relative Solar |
par5 |
redshift, z |
norm |
Mass accretion rate (solar mass/yr) |
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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.
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