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dc.contributor.authorTamura, M.
dc.contributor.authorHayashi, S.
dc.contributor.authorHough, J.
dc.identifier.citationTamura , M , Hayashi , S & Hough , J 1995 , ' Millimeter polarimetry of star-forming regions : magnetic field structure and low mass stars ' , Astrophysics and Space Science , vol. 224 , no. 1-2 , pp. 21-24 .
dc.identifier.otherPURE: 170533
dc.identifier.otherPURE UUID: 0c2b5b9a-970f-4a80-a459-a1b404b315d1
dc.identifier.otherdspace: 2299/3259
dc.identifier.otherScopus: 34249756399
dc.description“The original publication is available at”. Copyright Springer. DOI: 10.1007/BF00667815 [Full text of this article is not available in the UHRA]
dc.description.abstractWe have measured polarization of the 1.1 mm and 0.8 mm continuum emission for 3 pre-T Tauri stars and 2 T Tauri stars. Positive detections were made for NGC 1333 IRAS 4 and IRAS 16293-2422, while L1551 IRS 5 and HL Tau were only marginally detected. For GG Tau we measured a 2? upper limit of 3%. The polarization is interpreted in terms of thermal emission by magnetically aligned dust grains in circumstellar disks or envelopes. We have found a definite geometrical relation between the polarization and other circumstellar structure.en
dc.relation.ispartofAstrophysics and Space Science
dc.subjectcircumstellar disks
dc.titleMillimeter polarimetry of star-forming regions : magnetic field structure and low mass starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review

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