dc.contributor.author | Tamura, M. | |
dc.contributor.author | Hayashi, S. | |
dc.contributor.author | Hough, J. | |
dc.date.accessioned | 2009-04-22T08:11:14Z | |
dc.date.available | 2009-04-22T08:11:14Z | |
dc.date.issued | 1995 | |
dc.identifier.citation | Tamura , 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 . https://doi.org/10.1007/BF00667815 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.other | dspace: 2299/3259 | |
dc.identifier.uri | http://hdl.handle.net/2299/3259 | |
dc.description | “The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1007/BF00667815 [Full text of this article is not available in the UHRA] | |
dc.description.abstract | We 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.language.iso | eng | |
dc.relation.ispartof | Astrophysics and Space Science | |
dc.subject | circumstellar disks | |
dc.title | Millimeter polarimetry of star-forming regions : magnetic field structure and low mass stars | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1007/BF00667815 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |