  We present the orbital and physical parameters of the detached eclipsing
binary V1200~Centauri (ASAS~J135218-3837.3) from the analysis of spectroscopic
observations and light curves from the \textit{All Sky Automated Survey} (ASAS)
and SuperWASP database. The radial velocities were computed from the
high-resolution spectra obtained with the OUC 50-cm telescope and PUCHEROS
spectrograph and with 1.2m Euler telescope and CORALIE spectrograph using the
cross-correlation technique \textsc{todcor}. We found that the absolute
parameters of the system are $M_1= 1.394\pm 0.030$ M$_\odot$, $M_2= 0.866\pm
0.015$ M$_\odot$, $R_1= 1.39\pm 0.15$ R$_\odot$, $R_2= 1.10\pm 0.25$ R$_\odot$.
We investigated the evolutionary status and kinematics of the binary and our
results indicate that V1200~Centauri is likely a member of the Hyades moving
group, but the largely inflated secondary's radius may suggest that the system
may be even younger, around 30 Myr. We also found that the eclipsing pair is
orbited by another, stellar-mass object on a 351-day orbit, which is unusually
short for hierarchical triples. This makes V1200 Cen a potentially interesting
target for testing the formation models of multiple stars.
