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25 GHz methanol masers in regions of massive star formation

  • Tui R. Britton (a1) (a2) and Maxim A. Voronkov (a2)
  • DOI: http://dx.doi.org/10.1017/S1743921312007144
  • Published online: 01 July 2012
Abstract
Abstract

The bright 25 GHz series of methanol masers is formed in highly energetic regions of massive star formation and provides a natural signpost of shocked gas surrounding newly forming stars. A systematic survey for the 25 GHz masers has only recently been carried out. We present the preliminary results from the interferometric follow up of 51 masers at 25 GHz in the southern sky.

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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.

S. Kurtz , P. Hofner & C. V. Álvarez 2004, ApJS, 155, 149

R. L. Plambeck & K. M. Menten 1990, ApJ, 364, 555

M. A. Voronkov , K. J. Brooks , A. M. Sobolev , S. P. Ellingsen , A. B. Ostrovskii , & J. L. Caswell 2006, MNRAS, 373, 411

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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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