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Masers in G34.3+0.2: What more can 6.7-GHz methanol masers tell us?
Published online by Cambridge University Press: 03 August 2017
Abstract
We present results of 6.7 GHz methanol maser observations using the European VLBI Network (EVN) toward the G34.3+0.2 complex, which contains a prototypical cometary HII region and a dust enshrouded, probably emerging massive star, G34.24+0.13. We have investigated the methanol maser distribution in both objects and compared it with the OH and water masers in the main HII region. The masers in G34.24+0.13 lie on top of the 1.3 mm continuum emission showing that methanol masers are present, even at this early evolutionary stage.
- Type
- Part 1. Star Formation
- Information
- Symposium - International Astronomical Union , Volume 206: Cosmic Masers: From Protostars to Blackholes , 2002 , pp. 159 - 162
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
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