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.
|Title of host publication||Cosmic Masers - from OH to H0|
|Editors||Roy S. Booth, Elizabeth M. L. Humphreys, Wouter H. T. Vlemmings|
|Place of Publication||Cambridge|
|Publisher||Cambridge University Press|
|Number of pages||2|
|Publication status||Published - Jul 2012|
|Name||Proceedings of the International Astronomical Union|