dc.contributor.author | Lowe, K. | |
dc.contributor.author | Gledhill, T. | |
dc.date.accessioned | 2008-01-30T10:36:09Z | |
dc.date.available | 2008-01-30T10:36:09Z | |
dc.date.issued | 2005 | |
dc.identifier.citation | Lowe , K & Gledhill , T 2005 , Near Infrared Polarimetry of IRAS 19306+1407 . in In: Astronomical Polarimetry: Current Status and Future Directions - ASP Conf Series 343 . Astronomical Society of the Pacific , pp. 282-3 . | |
dc.identifier.isbn | 978-1-58381-277-8 | |
dc.identifier.isbn | 1-58381-210-5 | |
dc.identifier.other | dspace: 2299/1431 | |
dc.identifier.other | ORCID: /0000-0002-2859-4600/work/30779771 | |
dc.identifier.uri | http://hdl.handle.net/2299/1431 | |
dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical Society of the Pacific | |
dc.description.abstract | Polarimetry can be used to observe the dusty outer shells of Post- AGB stars. We can discriminate between the unpolarized light from the central star and the re°ected polarized °ux. The polarisation vectors and polarized °ux can give valuable information on the morphology of the object and the dust grain size distribution. Here we present J and K waveband polarimetry information and modeling of IRAS 19306+1407. We have detected scattered light and high degrees of linear polarisation. In polarized °ux we have detected a `dumbbell' structure, possibly indicating a detached dusty circumstellar envelope (CSE).We have constructed a light scattering model that includes polarisation to investigate the CSE structure in detail. | en |
dc.format.extent | 224197 | |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Astronomical Polarimetry: Current Status and Future Directions - ASP Conf Series 343 | |
dc.title | Near Infrared Polarimetry of IRAS 19306+1407 | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |