Polarization studies of nebulae associated with young stars and outflow regions

Details Polarization studies of nebulae associated with young stars and outflow regions Polarization studies of nebulae associated with young stars and outflow regions

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990qjras..31...47s&link_type=abstract

Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 31, March 1990, p. 47-52.

Astronomy and Astrophysics

Astronomy

14

Accretion Disks, Early Stars, Optical Polarization, Reflection Nebulae, Star Formation, Cosmic Dust, Interstellar Gas, Stellar Envelopes

Scientific paper

Consideration is given to the polarization disks observed in optical polarization maps of the central regions of reflection nebulae associated with young stars and outflows. Several models to explain the origin of polarization disks are reviewed, including multiple scattering models, the polarized source model, and the magnetized disk model. It is suggested that the properties of polarization disks can be explained by a hybrid of the polarized source and the magnetized disk models.

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