Open Access

Table 4

Parameters of ten Galactic clusters in the direction of the anticenter with polarization measurements from our observations and the literature.

Cluster b dis P σPav${\sigma _{{P_{av}}}}$ θ σθav${\sigma _{{\theta _{av}}}}$ Members Reference for polarization measurements
(deg) (deg) (kpc) (%) (%) (deg) (deg)
Kronberger 1 173.106 0.049 2.12 2.55 0.61 −27.2 4.9 19 This work
Berkeley 69 174.442 −1.851 3.18 3.23 0.70 −33.8 8.7 48 This work
Berkeley 71 176.635 0.901 3.50 1.50 0.53 −40.0 15.5 28 This work
King 8 176.384 3.104 4.79 3.13 0.99 −25.8 7.2 38 This work
Berkeley 19 176.919 −3.612 5.25 1.08 0.27 −62.5 14.9 04 This work
NGC 2281 174.892 16.889 0.51 0.85 0.14 16.6 4.8 09 1
NGC 1960 174.544 1.076 1.12 1.23 0.12 −21.3 4.7 08 1
Stock 8 173.375 −0.190 1.96 2.60 0.53 −25.1 7.0 05 1
NGC 1931 173.914 0.269 2.11 1.85 1.39 −25.4 9.4 18 2
NGC1 1893 173.582 −1.659 2.85 2.70 0.33 −21.9 4.7 22 3

Notes. The cluster parameters include the cluster distance (dis), the average degree of polarization (P), and the polarization angle (θ), calculated as the mean values of the corresponding parameters for member stars. σ and є represent the dispersion and propagated uncertainty in the polarization measurements for the member stars. (1) Eswaraiah et al. (2011); (2) Pandey et al. (2013); (3) Bijas et al. (2022).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.