Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7316
Title: Polarization of seven MBM clouds at high Galactic latitude
Authors: Neha, S
Maheswar, G
Soam, A
Lee, C. W
Keywords: Polarization;ISM: clouds;ISM: individual objects: MBM 33-39;ISM: magnetic fields
Issue Date: Jun-2018
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 476, No. 4, pp.4442-4458
Abstract: We made R-band polarization measurements of 234 stars towards the direction of the MBM 33-39 cloud complex. The distance of the MBM 33-39 complex was determined as 120 ± 10 pc using polarization results and near-infrared photometry from the 2MASS survey. The magnetic field geometry of the individual clouds inferred from our polarimetric results reveals that the field lines are in general consistent with the global magnetic field geometry of the region obtained from previous studies. This implies that the clouds in the complex are permeated by the interstellar magnetic field. Multi-wavelength polarization measurements of a few stars projected on to the complex suggest that the size of the dust grains in these clouds is similar to those found in the normal interstellar medium of the Milky Way. We studied a possible formation scenario of the MBM 33-39 complex by combining the polarization results from our study with those from the literature and by identifying the distribution of ionized, atomic and molecular (dust) components of material in the region.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7316
ISSN: 1365-2966
???metadata.dc.rights???: © Royal Astronomical Society
???metadata.dc.relation.uri???: https://doi.org/10.1093/mnras/sty485
Appears in Collections:IIAP Publications

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