  We present a study of the X-ray coronal emission from the active binary VY
Ari, using data from both the Low Energy Concentrator Spectrometer (LECS) and
the Medium Energy Concentrator Spectrometer (MECS) instruments on-board the
X-ray satellite BeppoSAX. Using these instruments, the X-ray spectrum of VY Ari
can be studied across two full decades of energy, from 0.1 to 10 keV. The
spectrum is well fit, across the whole spectral range, with an optically thin
plasma MEKAL model with two discrete temperature components, and with an
inferred coronal abundance $\feh \simeq -0.4$, corresponding to the average
typical value of the photospheric abundance in RS CVn-type binaries.
