Scattered OH maser sources in the direction of W49N

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4147

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DC Field	Value	Language
dc.contributor.author	Mendoza-Torres, Jose E.	-
dc.contributor.author	Goss, W.M.	-
dc.contributor.author	Streb, S.	-
dc.contributor.author	Deshpande, A.A.	-
dc.contributor.author	Ramachandran, R.	-
dc.date.accessioned	2011-08-24T05:51:39Z	-
dc.date.available	2011-08-24T05:51:39Z	-
dc.date.issued	2009-04	-
dc.identifier.citation	IAU Symposium, 2009, Vol.259, p95	en
dc.identifier.uri	http://hdl.handle.net/2289/4147	-
dc.description	Restricted Access. Proceedings of the International Astronomical Union, IAU Symposium on Cosmic Magnetic Fields: From Planets, 2009.	en
dc.description.abstract	OH 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.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2009IAUS..259...95M	en
dc.relation.uri	http://dx.doi.org/10.1017/S1743921309030142	en
dc.rights	2009 International Astronomical Union.	en
dc.title	Scattered OH maser sources in the direction of W49N	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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