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What is happening in G357.96-0.16?

Published online by Cambridge University Press:  24 July 2012

Tui R. Britton ,
Maxim A. Voronkov  and
Vanessa A. Moss
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
Maxim A. Voronkov
Affiliation:
CSIRO Astronomy & Space Science, PO Box 76, Epping, NSW 1710, Australia
Vanessa A. Moss
Affiliation:
CSIRO Astronomy & Space Science, PO Box 76, Epping, NSW 1710, Australia SIfA, School of Physics, University of Sydney, NSW 2006, Australia
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Abstract

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In order to answer this question, we examine the relationship between the two sites of maser activity in G357.96-0.16. We also propose future observations for examining the dust properties of this interesting region of massive star formation.

Keywords

masersstars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S287: Cosmic Masers - from OH to H0 , January 2012 , pp. 176 - 177
Copyright
Copyright © International Astronomical Union 2012

References

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