Polarimetry of young stellar objects - III. Circular polarimetry of OMC-1

Citation
A. Chrysostomou et al., Polarimetry of young stellar objects - III. Circular polarimetry of OMC-1, M NOT R AST, 312(1), 2000, pp. 103-115
Citations number
35
Categorie Soggetti
Space Sciences
Journal title
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN journal
00358711 → ACNP
Volume
312
Issue
1
Year of publication
2000
Pages
103 - 115
Database
ISI
SICI code
0035-8711(20000211)312:1<103:POYSO->2.0.ZU;2-I
Abstract
We present the first imaging circular polarimetry of the Orion Molecular Cl oud, OMC-1. The observations, taken in the J, H, K-n and nbL bands, reveal a complex pattern of circular polarization. Globally, there is a background circular polarization of the order of +/- 2 per cent in the K-n band, conf orming to the typical quadrupolar patterns that have been observed in other outflow sources. Overlying this pattern are regions of relatively high deg rees of circular polarization to the east and west of the source IRc2, with degrees as high as +17 per cent in the K-n band, the highest circular pola rization yet measured for any young stellar object. No circular polarizatio n is seen in the J band, indicating that the circular polarization detected at longer wavelengths originates from within OMC-1 and not from scattering off the foreground ionization front associated with the M42 nebula. We demonstrate a correlation between these patches of high circular polariz ation and regions of enhanced linear polarization, and argue that these obs ervations are best explained using a model that incorporates scattering of radiation off oblate grains, which have been aligned by the local magnetic field. Modelling of the ellipticity (the ratio of circular to linear polari zation) suggests that the grains are composed of silicate and/or organic re fractory material, and that grains larger than are typically found in the i nterstellar medium are needed. The lower, background, circular polarization is produced by scattering off randomly oriented grains in the outflow cavi ties, the grain alignment being destroyed by the passage of shocks. We put forward a morphological model for OMC-1 which has the regions of hig h polarization separate from, but near to, the main outflow region. Those r egions exhibiting high polarization must somehow have a direct view of the illuminating source of the nebula. Implications of this work to the origins of life are briefly discussed.