dc.contributor.author | Curran, R. | |
dc.contributor.author | Chrysostomou, A. | |
dc.contributor.author | Collett, J. | |
dc.contributor.author | Aitken, D. | |
dc.contributor.author | Jenness, T. | |
dc.date.accessioned | 2008-02-21T10:55:11Z | |
dc.date.available | 2008-02-21T10:55:11Z | |
dc.date.issued | 2005 | |
dc.identifier.citation | Curran , R , Chrysostomou , A , Collett , J , Aitken , D & Jenness , T 2005 , First SCUBA Polarimetry of Two Candidate High-Mass Protostellar Objects . in In: Astronomical Polarimetry: Current Status and Future Directions, ASP Conference Series 343 . Astronomical Society of the Pacific , pp. 185-186 . | |
dc.identifier.other | dspace: 2299/1672 | |
dc.identifier.uri | http://hdl.handle.net/2299/1672 | |
dc.description | Original paper can be found at: http://aspbooks.org/custom/publications/paper/343-0185.html Copyright Astronomical Society of the Pacific | |
dc.description.abstract | We present the first polarimetry towards two candidate highmass protostellar objects - W48W and S152SE. The polarimetry across both candidate HMPOs is ordered with a high degree of polarization (6-8%) compared to that of the nearby HII regions. Plane-of-the-sky magnetic field strengths of 0.7mG for W48W and 0.2mG for S152SE have been calculated using the Chandrasekhar-Fermi (CF) method, and mass-to-magnetic flux ratios indicate that both of these clouds are close to the critical value. | en |
dc.format.extent | 179320 | |
dc.language.iso | eng | |
dc.publisher | Astronomical Society of the Pacific | |
dc.relation.ispartof | In: Astronomical Polarimetry: Current Status and Future Directions, ASP Conference Series 343 | |
dc.title | First SCUBA Polarimetry of Two Candidate High-Mass Protostellar Objects | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Science & Technology Research Institute | |
dc.contributor.institution | Centre for Astrophysics Research | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |