  Stellar coronal sources have been observed in the past not only for their
astrophysical interest in the field of binary system evolution and interaction,
but also for their invaluable roles as benchmarks for plasma spectral models
and as calibration sources for high resolution spectroscopic X-ray instruments.
These include the gratings on-board Chandra and XMM-Newton, as well as the new
generation of high resolution capable-detectors recently flown on-board XRISM
and planned for the future also on-board the Athena and the LEM missions. In
our previous paper exploiting Chandra/HETG observations of the prototypical
coronal source Capella, it has been shown that the centroid energies of the
many X-ray emission lines detected in the spectrum of this object change as a
function of time due to the Doppler modulation within the binary. This is an
effect that needs to be corrected while performing calibrations of high
resolution X-ray instruments. In this paper, we extend our previous work on
Capella to other known stellar coronal sources which have been observed with
the Chandra/HETG (11 objects in total). We measure in several objects clear
trends in the velocity shifts along the orbit of the primary star, meaning that
in these sources one of the two star components is largely dominating the high
energy emission. In a number of systems the trend in the velocity shift is not
obvious. This can be ascribed to the fact that both stellar components
contribute significantly to the X-ray emission.
