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Interstellar polarization: Magnetite dust

Journal Article · · Astrophys. J., v. 201, no. 1, pp. 151-164
DOI:https://doi.org/10.1086/153868· OSTI ID:4098971
The polarization and extinction properties of magnetite, or Fe$sub 3$$O$$sub 4$, dust grains are calculated based on indirect evidence that magnetite grains might be the interstellar polarizers. The extinction and phase-lag cross sections of magnetite grains are calculated using a computer method for nonspherical grains. From these, the linear and circular polarization which would be produced by a medium of aligned magnetite dust grains is determined. It is found that flat platelets of magnetite can reproduce the wavelength dependence of the polarization observations. Furthermore, given the predictions by the Purcell ''pinwheel'' alignment mechanism of perfect alignment for such grains, it is shown that magnetite grains can produce all the observed polarization at the visual wavelength by consuming roughly 16 percent of the cosmic abundance of iron atoms in the interstellar medium, while contributing roughly 4 percent of the total visual extinction. With less than perfect alignment, more iron must be put into the magnetite grains, resulting in more magnetite extinction. A general property of interstellar polarization is also discussed based on the Kramers-- Kronig dispersion relations. An infrared observational test of property is proposed. (AIP)
Research Organization:
Center for Astrophysics, Harvard College Observatory and Smithsonian Astrophysical Observatory
Sponsoring Organization:
USDOE
NSA Number:
NSA-33-018174
OSTI ID:
4098971
Journal Information:
Astrophys. J., v. 201, no. 1, pp. 151-164, Journal Name: Astrophys. J., v. 201, no. 1, pp. 151-164; ISSN ASJOA
Country of Publication:
United States
Language:
English

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