BVIC photometry and classification spectroscopy is presented for the young
open cluster NGC 6604. Additional Echelle spectroscopy of the brightest mem
bers is used to check the reddening against the interstellar NaI and KI abs
orption lines, to measure the cluster radial velocity and to derive the ind
ividual rotational velocities. We obtain 1.7 kpc as the cluster distance, a
n age of similar to 5 10(6) years and a reddening EB-V= 1.02 (+/-0.01 from
three independent methods). Pre-ZAMS objects are apparently not detected ov
er the Delta m = 8.5 mag explored range. The cluster radial velocity is in
agreement with the Hron (1987) model for the Galaxy disk rotation.