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Magnetic fields in multiple bright-rimmed clouds in different directions of H II region IC 1396

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dc.contributor.author Soam, A
dc.contributor.author Maheswar, G
dc.contributor.author Lee, C. W
dc.contributor.author Neha, S
dc.contributor.author Kim, K
dc.date.accessioned 2020-11-10T02:40:37Z
dc.date.available 2020-11-10T02:40:37Z
dc.date.issued 2018-06
dc.identifier.citation Monthly Notices of the Royal Astronomical Society, Vol. 476, No. 4, pp. 4782-4793 en_US
dc.identifier.issn 1365-2966
dc.identifier.uri http://prints.iiap.res.in/handle/2248/6756
dc.description Restricted Access © Royal Astronomical Society; https://doi.org/10.1093/mnras/sty517 en_US
dc.description.abstract Bright-rimmed clouds (BRCs) form on the edges of H II regions affected by high-energy radiation from a central ionizing source. The UV radiation from the ionizing source results in compression and ionization, causing either cloud disruption or further star formation. In this work, we present R-band polarization measurements towards four BRCs, namely IC 1396A, BRC  37, BRC 38 and BRC 39, located in different directions in the H II region, Sh2-131, in order to map the magnetic field (B-field) in the plane of the sky. These BRCs are illuminated by the O star HD 206267 and present a range of projected on-sky geometries. This provides an opportunity to gain an understanding of the magnetized evolution of BRCs. The B-field geometries of the clouds deduced from the polarization data, after correction for foreground contamination by the interstellar medium, are seen to be connected to the ambient B-fields on large scales. They seem to play an important role in shaping the clouds IC 1396A and BRC 37. BRCs 38 and 39 show a broader and snubber head morphology, possibly because the B-fields are aligned with incoming radiation, as revealed in the simulations. A good general agreement is noted on comparing our observational results with the simulations, supporting the importance of B-fields in BRC evolution. This work is the first step towards systematic mapping the B-fields morphology in multiple BRCs in an expanding H II region, extending our previous work. en_US
dc.language.iso en en_US
dc.publisher Oxford University Press on behalf of the Royal Astronomical Society en_US
dc.subject Polarization en_US
dc.subject ISM: clouds en_US
dc.subject Dust en_US
dc.subject Extinction en_US
dc.subject H II regions en_US
dc.subject ISM: magnetic fields en_US
dc.title Magnetic fields in multiple bright-rimmed clouds in different directions of H II region IC 1396 en_US
dc.type Article en_US

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