dc.contributor.author | Aitken, D. | |
dc.contributor.author | Bailey, J. | |
dc.contributor.author | Roche, P.F. | |
dc.contributor.author | Hough, J. | |
dc.date.accessioned | 2009-04-20T13:58:43Z | |
dc.date.available | 2009-04-20T13:58:43Z | |
dc.date.issued | 1985 | |
dc.identifier.citation | Aitken , D , Bailey , J , Roche , P F & Hough , J 1985 , ' Infrared spectropolarimetric observations of BNKL : the grain alignment mechanism ' , Monthly Notices of the Royal Astronomical Society , vol. 215 , no. 4 , pp. 815-831 . | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.other | dspace: 2299/3227 | |
dc.identifier.uri | http://hdl.handle.net/2299/3227 | |
dc.description | Original article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA] | |
dc.description.abstract | Spectropolarimetric observations between 8 - 13 μm of BN, IRc 2, 3, 4 and a further region in the Orion infrared complex BNKL are presented. Apart from IRc 2, all show evidence for absorption by aligned grains and have polarization position angles directed at a region close to IRc 2, a property also shared by the self-luminous source IRc 9 at short wavelengths. The evidence strongly suggests that grains are aligned by the intrinsic angular momentum of photons from IRc 2 and it is shown that this is a quantitatively plausible mechanism for the physical conditions in this part of Orion. | en |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | Infrared spectropolarimetric observations of BNKL : the grain alignment mechanism | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |