Please use this identifier to cite or link to this item:
|Title:||Maser Action in Methanol Transitions|
|Publisher:||Springer Science and Business Media LLC|
|Citation:||Maser Action in Methanol Transitions / M. Voronkov, A. Sobolev, S. Ellingsen et al. — DOI 10.1080/14697680802165736 // Astrophysics and Space Science. — 2005. — Vol. 295. — Iss. 1-2. — P. 217-223.|
|Abstract:||We report the detection with the ATCA of 6.7 GHz methanol emission towards OMC-1. The source has a size between 40″ and 90″, is located to the south-east of Ori-KL and may coincide in position with the 25 GHz masers. The source may be an example of an interesting case recently predicted in theory where the transitions of traditionally different methanol maser classes show maser activity simultaneously. In addition, results of recent search for methanol masers from the 25 and 104.3 GHz transitions are reported. © Springer 2005 Science + Business Media, Inc.|
|metadata.dc.description.sponsorship:||We would like to thank the local staff of Narrabri and Onsala observatories for the help during observations. The Australia Telescope is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. Maxim Voronkov and Alexei Alakoz were partially supported by the RFBR grant no. 01-02-16902 and by the program “Extended objects in the Universe-2003”. Andrej Sobolev and Andrei Ostrovskii were supported by the RFBR grant no. 03-02-16433.|
|Appears in Collections:||Научные публикации, проиндексированные в SCOPUS и WoS CC|
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.