English

Scattering polarization of 3-$\mu$m water-ice feature by large icy grains

Astrophysics of Galaxies 2021-03-31 v1 Earth and Planetary Astrophysics Solar and Stellar Astrophysics

Abstract

Water ice has a strong spectral feature at a wavelength of approximately 3 μ3~\mum, which plays a vital role in our understanding of the icy universe. In this study, we investigate the scattering polarization of this water-ice feature. The linear polarization degree of light scattered by μ\mum-sized icy grains is known to be enhanced at the ice band; however, the dependence of this polarization enhancement on various grain properties is unclear. We find that the enhanced polarization at the ice band is sensitive to the presence of μ\mum-sized grains as well as their ice abundance. We demonstrate that this enhancement is caused by the high absorbency of the water-ice feature, which attenuates internal scattering and renders the surface reflection dominant over internal scattering. Additionally, we compare our models with polarimetric observations of the low-mass protostar L1551 IRS 5. Our results show that scattering by a maximum grain radius of a few microns with a low water-ice abundance is consistent with observations. Thus, scattering polarization of the water-ice feature is a useful tool for characterizing ice properties in various astronomical environments.

Keywords

Cite

@article{arxiv.2101.07635,
  title  = {Scattering polarization of 3-$\mu$m water-ice feature by large icy grains},
  author = {Ryo Tazaki and Koji Murakawa and Takayuki Muto and Mitsuhiko Honda and Akio K. Inoue},
  journal= {arXiv preprint arXiv:2101.07635},
  year   = {2021}
}

Comments

19 pages, 17 figures, 1 table; Accepted for publication in ApJ