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Scattered OH maser sources in the direction of W49N

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dc.contributor.authorMendoza-Torres, Jose E
dc.contributor.authorGoss, W M
dc.contributor.authorStreb, S
dc.contributor.authorDeshpande, A A
dc.contributor.authorRamachandran, R
dc.date.accessioned2011-08-24T05:51:39Z
dc.date.available2011-08-24T05:51:39Z
dc.date.issued2009-04
dc.descriptionRestricted Access. Proceedings of the International Astronomical Union, IAU Symposium on Cosmic Magnetic Fields: From Planets, 2009.en
dc.description.abstractOH masers spots are observed with the VLBA at 1612, 1665 and 1667 MHz. The orientation of the ellipses resulting from scattering are all nearly aligned perpendicular to the galactic plane. These ordered orientation could be due to the galactic magnetic field.en
dc.identifier.citationIAU Symposium, 2009, Vol.259, p95en
dc.identifier.urihttp://hdl.handle.net/2289/4147
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.urihttp://adsabs.harvard.edu/abs/2009IAUS..259...95Men
dc.relation.urihttp://dx.doi.org/10.1017/S1743921309030142en
dc.rights2009 International Astronomical Union.en
dc.titleScattered OH maser sources in the direction of W49Nen
dc.typeArticleen

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