  A growing number of observations indicate that magnetic fields are present
among a small fraction of massive O- and B-type stars, yet the origin of these
fields remains unclear. Here we present the results of a VLT/FORS1
spectropolarimetric survey of 15 B-type members of the open cluster NGC 3766.
We have detected two magnetic B stars in the cluster, including one with a
large field of nearly 2 kG, and we find marginal detections of two additional
stars. There is no correlation between the observed longitudinal field
strengths and the projected rotational velocity, suggesting that a dynamo
origin for the fields is unlikely. We also use the Oblique Dipole Rotator model
to simulate populations of magnetic stars with uniform or slightly varying
magnetic flux on the ZAMS. None of the models successfully reproduces our
observed range in B_l and the expected number of field detections, and we rule
out a purely fossil origin for the observed fields.
