| dc.contributor.author | Hough, J. | |
| dc.contributor.author | Bailey, J. | |
| dc.contributor.author | Cunningham, E.C. | |
| dc.contributor.author | McCall, A. | |
| dc.date.accessioned | 2009-04-20T12:31:20Z | |
| dc.date.available | 2009-04-20T12:31:20Z | |
| dc.date.issued | 1981 | |
| dc.identifier.citation | Hough , J , Bailey , J , Cunningham , E C & McCall , A 1981 , ' Linear polarization of T-Tauri stars ' , Monthly Notices of the Royal Astronomical Society , vol. 195 , no. 2 , pp. 429-436 . | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | PURE: 165931 | |
| dc.identifier.other | PURE UUID: 6ae8285c-059e-4fde-9785-208fd7fc8143 | |
| dc.identifier.other | dspace: 2299/3218 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3218 | |
| 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 | Linear polarization observations over the wavelength range 0.44-2.2 microns are presented for six T Tauri type stars. All of the stars studied show substantial polarization in the infrared, while T Tau itself (and probably SU Aur) show a 90 deg change in position angle in the infrared. The data are discussed in terms of scattering from circumstellar dust grains with a component of large (approximately 1 micron) grains being required to fit the observed spectral dependence. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | Linear polarization of T-Tauri stars | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
