Interstellar extinction, polarization, and grain alignment in the Sh 2-185 (IC 59 and IC 63) region

Abstract

Optical and infrared continuum polarization from the interstellar medium is driven by radiative processes aligning the grains with the magnetic field. While a quantitative, predictive theory of Radiative Alignment Torques (RAT) exists and has been extensively tested, several parameters of the theory remain to be fully constrained. In a recent paper, \citet{medan2019} showed that the polarization efficiency (and therefore grain alignment efficiency) at different locations in the wall of the Local Bubble (LB) could be modeled as proportional to the integrated light intensity from the surrounding stars and OB associations. Here we probe that relationship at high radiation field intensities by studying the extinction and polarization in the two reflection nebulae IC\,59 and IC\,63 in the Sh 2-185 H II region, illuminated by the B0 IV star $\gamma$ Cassiopeia. We combine archival visual polarimetry with new 7-band photometry in the Vilnius system, to derive the polarization efficiency from the material. We find that the same linear relationship seen in the Local Bubble wall also applies to the Sh 2-185 region, strengthening the conclusion from the earlier study.

arXiv comment31 pages, 11 figures, 4 tables (data under tables will be uploaded to CDS), Accepted for publication in AJ

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• SOFIA observations of 30 Doradus: I -- Far-Infrared dust polarization and implications for grain alignment and disruption by radiative torques
• Nano-grain depletion in photon-dominated regions
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• Core orientations and magnetic fields in isolated molecular clouds
• High Resolution Observations of HI in the IC 63 Reflection Nebula
• Physics and Chemistry of Radiation Driven Cloud Evolution. [C II] Kinematics of IC 59 and IC 63
• Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective