NGC 7067 is a young open cluster located in the direction between the first and the second Galactic quadrants and close to the Perseus spiral arm .
This makes it useful for studies of the nature of the Milky Way spiral arms .
Strömgren photometry taken with the Wide Field Camera at the Isaac Newton Telescope allowed us to compute individual physical parameters for the observed stars and hence to derive cluster ’ s physical parameters .
Spectra from the 1.93-m telescope at the Observatoire de Haute-Provence helped to check and improve the results .
We obtained photometry for 1233 stars , individual physical parameters for 515 and spectra for 9 of them .
The 139 selected cluster members lead to a cluster distance of 4.4 \pm 0.4 kpc , with an age below \log _ { 10 } ( t ( \mathrm { yr } ) ) = 7.3 and a present Mass of 1260 \pm 160 \mathrm { M } _ { \sun } .
The morphology of the data reveals that the centre of the cluster is at ( \alpha, \delta ) = ( 21 \colon 24 \colon 13.69 , +48 \colon 00 \colon 39.2 ) J2000 , with a radius of 6 \farcm 1 .
Strömgren and spectroscopic data allowed us to improve the previous parameters available for the cluster in the literature .