| dc.contributor.author | Mead, A.R.G. | |
| dc.contributor.author | Brand, P.W.J.L. | |
| dc.contributor.author | Hough, J. | |
| dc.contributor.author | Bailey, J. | |
| dc.date.accessioned | 2009-04-20T08:08:19Z | |
| dc.date.available | 2009-04-20T08:08:19Z | |
| dc.date.issued | 1988 | |
| dc.identifier.citation | Mead , A R G , Brand , P W J L , Hough , J & Bailey , J 1988 , ' Polarimetric observations of the quasar 3C-345 ' , Monthly Notices of the Royal Astronomical Society , vol. 233 , no. 2 , pp. 503-509 . | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | PURE: 153067 | |
| dc.identifier.other | PURE UUID: f2ebbe65-64e5-457f-971a-a4e3dc803844 | |
| dc.identifier.other | dspace: 2299/3206 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3206 | |
| 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 | Infrared and optical polarimetric observations of the quasar 3C 345 are presented, which show a decrease in the degree of polarization with frequency previously observed by Smith et al., and interpreted by them as the result of dilution of the polarized flux by a non-polarized thermal component (the "blue bump"). The new data are compared to previous fits of this model to 3C 345, and the validity of the model is discussed. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.subject | astronomic models | |
| dc.subject | Balmer series | |
| dc.subject | black body radiation | |
| dc.subject | emission spectra | |
| dc.title | Polarimetric observations of the quasar 3C-345 | 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 | |
