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dc.contributor.authorMacquart, Jean-pierre
dc.contributor.authorBower, G.
dc.contributor.authorWright, M.
dc.contributor.authorBacker, D.
dc.contributor.authorFalcke, H.
dc.date.accessioned2017-01-30T10:45:59Z
dc.date.available2017-01-30T10:45:59Z
dc.date.created2010-03-23T20:02:56Z
dc.date.issued2006
dc.identifier.citationMacquart, Jean-pierre and Bower, G and Wright, Melvyn and Backer, Donald and Falcke, Heino. 2006. The Rotation Measure and 3.5 Millimeter Polarization of Sagittarius A*. The Astrophysical Journal. 646: pp. L111-L114.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/5420
dc.identifier.doi10.1086/506932
dc.description.abstract

We report the detection of variable linear polarization from Sgr A* at a wavelength of 3.5 mm, the longest wavelength yet at which a detection has been made. The mean polarization is 2.1% 0.1% at a position angle of 162 with rms scatters of 0.4% and 9 over the five epochs. We also detect polarization variability on a timescale of days. Combined with previous detections over the range 150-400 GHz (750-2000 mm), the average polarization position angles are all found to be consistent with a rotation measure of (4.40.3)#105 rad m2. This implies that the Faraday rotation occurs external to the polarized source at all wavelengths. This implies an accretion rate ~(0.2-4)#108 M, yr1 for the accretion density profiles expected of ADAF, jet, and CDAF models and assuming that the region at which electrons in the accretion flow become relativistic is within 10RS. The inferred accretion rate is inconsistent with ADAF/Bondi accretion. The stability of the mean polarization position angle between disparate polarization observations over the frequency range limits fluctuations in the accretion rate to less than 5%. The flat frequency dependence of the interday polarization position angle variations also makes them difficult to attribute to rotation-measure fluctuations and suggests that both the magnitude and position angle variations are intrinsic to the emission.

dc.publisherThe American Astronomical Society
dc.subjectmechanisms nonthermal
dc.subjectactive-Galaxy
dc.subjectgalaxies
dc.subjectcenter-polarization-radiation
dc.titleThe Rotation Measure and 3.5 Millimeter Polarization of Sagittarius A*
dc.typeJournal Article
dcterms.source.volume646
dcterms.source.startPageL111
dcterms.source.endPageL114
dcterms.source.issn0004637X
dcterms.source.titleThe Astrophysical Journal
curtin.note

Copyright © 2006 The American Astronomical Society ("AAS")-[The Astrophysical Journal (ApJ) Macquart, Jean-pierre, 2006 ApJS 646, L111-L114.]

curtin.accessStatusOpen access via publisher
curtin.facultyFaculty of Science and Engineering
curtin.facultyCurtin Institute of Radio Astronomy


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