Astrophysics and Space Science

, Volume 43, Issue 2, pp 291–317

Orientation of cosmic dust grains

Authors

  • A. Z. Dolginov
    • A. F. Ioffe Physical-Technical Institute of Academy of Sciences of USSR
  • I. G. Mytrophanov
    • A. F. Ioffe Physical-Technical Institute of Academy of Sciences of USSR
Article

DOI: 10.1007/BF00640010

Cite this article as:
Dolginov, A.Z. & Mytrophanov, I.G. Astrophys Space Sci (1976) 43: 291. doi:10.1007/BF00640010

Abstract

Orientation of nonspherical cosmic dust grains is found in anisotropic corpuscular or radiative fluxes and in the presence of the magnetic field; cosmic grains being approximated by axially symmetric ellipsoids. A comparatively small twisting of grains is shown to cause differences in scattering right-hand and left-hand circularly polarized photons and growth of the angular momentum. If the period of the grain's angular momentum precession induced by the magnetic field is shorter than the time of orientation by corpuscular or radiative flux, distribution of grains' axes becomes symmetric relative to the magnetic lines. This orientation mechanism easily explains interstellar linear polarization observed in our Galaxy. The mechanisms of grains' orientation near the Becklin-Neugebauer infrared source, in the B 96 reflected cloud near RY Tau and in cometary heads are proposed.

Copyright information

© D. Reidel Publishing Company 1976