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25 GHz methanol masers in regions of massive star formation

Published online by Cambridge University Press:  24 July 2012

Tui R. Britton
Affiliation:
Dept. of Physics & Astronomy, Macquarie University, Sydney, NSW 2109, Australia email: tui.britton@csiro.au CSIRO Astronomy & Space Science, PO Box 76, Epping, NSW 1710, Australia email: maxim.voronkov@csiro.au
Maxim A. Voronkov
Affiliation:
CSIRO Astronomy & Space Science, PO Box 76, Epping, NSW 1710, Australia email: maxim.voronkov@csiro.au
Corresponding
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

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