Abstract:
We present multiwavelength linear polarimetric observations of 104 stars towards the region
of young open cluster NGC 6823. The polarization towards NGC 6823 is dominated by
foreground dust grains and we found evidence for the presence of several layers of dust
towards the line of sight. The first layer of dust is approximately located within 200 pc towards
the cluster, which is much closer to the Sun than the cluster itself (∼2.1 kpc). The radial
distribution of the position angles for the member stars is found to show a systematic change,
while the polarization is found to reduce towards the outer parts of the cluster and the average
position angle of the coronal region of the cluster is very close to the inclination of the Galactic
parallel (∼32◦). The size distribution of the grains within NGC 6823 is similar to those in the
general interstellar medium. The patchy distribution of foreground dust grains is suggested
to be mainly responsible for both differential reddening and polarization towards NGC 6823.
The majority of the observed stars do not show evidence of intrinsic polarization in their light.