  We present measurements of the Fe-K line for nine Seyfert I galaxies using
Chandra High Energy Transmission Grating Spectrometer (HETGS) data. The
centroid energies are narrowly dispersed (6.403 +/- 0.062 keV) and indicate an
origin of the line cores in cold matter. If {\it all} the lines in this sample
were the peaks of a relativistically broadened disk line, it would require
unrealistically fine tuning. However, at least three of the nine AGN clearly
show a complex Fe-K line with an underlying broad component, possibly from a
disk. In the others, an apparently narrow Fe-K line (even if it is resolved by
Chandra) may still be due to the peak of a disk line. To distinguish this
scenario from an origin in distant matter requires variability information.
