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dc.contributor.authorCurran, R.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorCollett, J.
dc.contributor.authorAitken, D.
dc.contributor.authorJenness, T.
dc.date.accessioned2008-02-21T10:55:11Z
dc.date.available2008-02-21T10:55:11Z
dc.date.issued2005
dc.identifier.citationCurran , 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.otherdspace: 2299/1672
dc.identifier.urihttp://hdl.handle.net/2299/1672
dc.descriptionOriginal paper can be found at: http://aspbooks.org/custom/publications/paper/343-0185.html Copyright Astronomical Society of the Pacific
dc.description.abstractWe 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.extent179320
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Astronomical Polarimetry: Current Status and Future Directions, ASP Conference Series 343
dc.titleFirst SCUBA Polarimetry of Two Candidate High-Mass Protostellar Objectsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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