|
Voronkov, MA and Caswell, JL and Ellingsen, SP and Sobolev, AM, New 9.9-GHz methanol masers, Monthly Notices of the Royal Astronomical Society, 405, (4) pp. 2471-2484. ISSN 0035-8711 (2010) [Refereed Article]
Copyright StatementThe definitive published version is available online at: http://interscience.wiley.com Official URL: http://interscience.wiley.com DOI: doi:10.1111/j.1365-2966.2010.16624.x AbstractThe Australia Telescope Compact Array has been used to make the first extensive search for the class I methanol masers at 9.9 GHz. In total, 48 regions of high-mass star formation were observed. In addition to masers in W33-Met (G12.80−0.19) and G343.12−0.06 (IRAS 16547−4247) which have already been reported in the literature, two new 9.9-GHz masers have been found towards G331.13−0.24 and G19.61−0.23. We have determined absolute positions (accurate to roughly a second of arc) for all the detected masers and suggest that some class I masers may be associated with shocks driven into molecular clouds by expanding HII regions. Our observations also imply that the evolutionary stage of a high-mass starforming region when the class I masers are present can outlast the stage when the class II masers at 6.7-GHz are detectable, and overlaps significantly with the stage when OH masers are active.
Repository Staff Only: item control page |
