Circular polarisation in star-forming regions: Possible implications for homochirality
Identifieur interne : 00BA51 ( Main/Exploration ); précédent : 00BA50; suivant : 00BA52Circular polarisation in star-forming regions: Possible implications for homochirality
Auteurs : J. H. Hough [Royaume-Uni] ; J. A. Bailey [Australie] ; A. Chrysostomou [Royaume-Uni] ; T. M. Gledhill [Royaume-Uni] ; P. W. Lucas [Royaume-Uni] ; M. Tamura [Japon] ; S. Clark [Royaume-Uni] ; J. Yates [Royaume-Uni] ; F. Menard [France]Source :
- Advances in Space Research [ 0273-1177 ] ; 2001.
English descriptors
- KwdEn :
- Amino acids, Astron, Astrophysical situations, Asymmetric photolysis, Bailey, Chiral, Chiral initiator, Chiral molecules, Chiral organics, Chrysostomou, Circular dichroism, Circular polarisation, Circularly, Circularly polarised, Crab nebula, Dust cloud, Dust clouds, Dust grains, Ehiral molecules, Elsevier science, Favourable cases, Gledhill, Gledhill mccall, Gray scale, Handedness, High degrees, Homochirality, Large degrees, Linear polarisation, Lower right, Magnetic field, Many organics, Maximum degree, Menard, More material, Nearby star, Organic molecules, Other hand, Planetary system, Polarisation, Polarisation observations, Polarised, Polarised radiation, Present life, Radiation field, Radio wavelengths, Same handedness, Several percent, Several tens, Short axis, Single handedness, Size distribution, Solar system, Spie proc, Star formation, Star formation process, Starforming regions, Synchrotron radiation, Tauri star, Total flux, Uvcpl, Wavelength, Wavelength dependence.
- Teeft :
- Amino acids, Astron, Astrophysical situations, Asymmetric photolysis, Bailey, Chiral, Chiral initiator, Chiral molecules, Chiral organics, Chrysostomou, Circular dichroism, Circular polarisation, Circularly, Circularly polarised, Crab nebula, Dust cloud, Dust clouds, Dust grains, Ehiral molecules, Elsevier science, Favourable cases, Gledhill, Gledhill mccall, Gray scale, Handedness, High degrees, Homochirality, Large degrees, Linear polarisation, Lower right, Magnetic field, Many organics, Maximum degree, Menard, More material, Nearby star, Organic molecules, Other hand, Planetary system, Polarisation, Polarisation observations, Polarised, Polarised radiation, Present life, Radiation field, Radio wavelengths, Same handedness, Several percent, Several tens, Short axis, Single handedness, Size distribution, Solar system, Spie proc, Star formation, Star formation process, Starforming regions, Synchrotron radiation, Tauri star, Total flux, Uvcpl, Wavelength, Wavelength dependence.
Abstract
Abstract: Our discovery of high degrees of circular polarisation in some star-forming regions provides an attractive mechanism for the origin of homochirality. The largest degrees of circular polarisation, so far observed at near-infrared wavelengths, are thought to arise from the scattering of stellar radiation from aligned dust grains and are calculated to extend down to UV wavelengths. The extent of the region where circularly polarised light (CPL) of a single handedness originates is very large, and it is likely that the whole of a planetary system would see a single handedness of CPL also.We present the observational data, models of the scattering that leads to the production of CPL, and a model for the origin of homochirality. We also discuss briefly future laboratory and space-based experiments.
Url:
DOI: 10.1016/S0273-1177(01)00063-1
Affiliations:
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<front><div type="abstract" xml:lang="en">Abstract: Our discovery of high degrees of circular polarisation in some star-forming regions provides an attractive mechanism for the origin of homochirality. The largest degrees of circular polarisation, so far observed at near-infrared wavelengths, are thought to arise from the scattering of stellar radiation from aligned dust grains and are calculated to extend down to UV wavelengths. The extent of the region where circularly polarised light (CPL) of a single handedness originates is very large, and it is likely that the whole of a planetary system would see a single handedness of CPL also.We present the observational data, models of the scattering that leads to the production of CPL, and a model for the origin of homochirality. We also discuss briefly future laboratory and space-based experiments.</div>
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