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Scattered OH Maser sources in the direction of W49N

  • Jose E. Mendoza-Torres (a1), W. M. Goss (a2), S. Streb (a3), A. A. Deshpande (a4) and R. Ramachandran (a5)...
Abstract
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.

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      Scattered OH Maser sources in the direction of W49N
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This list contains references from the content that can be linked to their source. For a full set of references and notes please see the PDF or HTML where available.

K. M. Desai , C. R. Gwinn , & P. J. Diamond 1994, Nature 372, 754

C. R. Gwinn , J. M. Moran , & M. Reid 1992, ApJ 393, 149

S. R. Kent & R. L. Mutel 1982, ApJ 263, 145

R. Narayan & W. B. Hubbard 1988, ApJ 325, 503

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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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