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H2 and methanol masers - outflow from the earliest stages of high-mass star formation?

Published online by Cambridge University Press:  03 August 2017

J.-K. Lee
Affiliation:
School of Physics, The University of New South Wales, Sydney, NSW 2052, Australia
A.J. Walsh
Affiliation:
Max-Planck-Institut für Radioastronomie, auf dem Hügel 69, Bonn D-53121, Germany
M.G. Burton
Affiliation:
School of Physics, The University of New South Wales, Sydney, NSW 2052, Australia

Abstract

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We report the discovery of shocked H2 emission at 2.12 μm associated with methanol masers, and discuss its implication for massive star formation.

Type
Part 1. Star Formation
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

Ryder, S. D., Sun, Y.-S., Ashley, M. C. B., Burton, M. G., Allen, L. E., Storey, J. W. V., 1998, Proc. Astron. Soc. Aust., 15, 228 CrossRefGoogle Scholar
Ellingsen, S., Norris, R., McCulloch, P., 1996, MNRAS, 279, 101 CrossRefGoogle Scholar
Lee, J.-K., Walsh, A. J., Burton, M. G., Ashley, M. C. B., 2001, MNRAS, 324, 1102 CrossRefGoogle Scholar
Walsh, A. J., Hyland, A. R., Robinson, G., Burton, M. G., 1997, MNRAS, 291, 261 CrossRefGoogle Scholar
Walsh, A. J., Burton, M. G., Hyland, A. R., Robinson, G., 1998, MNRAS, 301, 640 CrossRefGoogle Scholar