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Samal, Saurabh Sharma, Shih-Ping Lai, Yuehui Ma, Zhiwei Chen","submitted_at":"2018-12-21T02:45:54Z","abstract_excerpt":"We present the results based on the optical $R$-band polarization observations of 280 stars distributed towards the dark globule LDN\\,1225. {\\it Gaia} data release 2 parallaxes along with the polarization data of $\\sim$200 stars have been used to (a) constrain the distance of LDN\\,1225 as 830$\\pm$83~pc, (b) determine the contribution of interstellar polarization (ISP), and (c) characterize the dust properties and delineate the magnetic field (B-field) morphology of LDN\\,1225. We find that B-fields are more organized and exhibit a small dispersion of 12$\\degr$. 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