113 citations · 137 across the 3 of their papers we have counts for
7 papers
How do methanol masers manage to appear in the youngest star vicinities and isolated molecular clumps?
A. M. Sobolev, D. M. Cragg, S. P. Ellingsen +10
General characteristics of methanol (CH3OH) maser emission are summarized. It is shown that methanol maser sources are concentrated in the spiral arms. Most of the methanol maser s…
The Australia Telescope campaign to study southern class I methanol masers
M. A. Voronkov, K. J. Brooks, A. M. Sobolev +3
The Australia Telescope Compact Array (ATCA) and the Mopra facility have been used to search for new southern class I methanol masers at 9.9, 25 (J=5) and 104 GHz, which are though…
Class I methanol masers in the outflow of IRAS 16547-4247
M. A. Voronkov, K. J. Brooks, A. M. Sobolev +3
The Australia Telescope Compact Array (ATCA) has been used to image class I methanol masers at 9.9, 25 (a series from J=2 to J=9), 84, 95 and 104 GHz located in the vicinity of IRA…
Methanol Masers and Star Formation
A. M. Sobolev, A. B. Ostrovskii, M. S. Kirsanova +3
Methanol masers which are traditionally divided into two classes provide possibility to study important parts of the star forming regions: Class~II masers trace vicinities of the m…
The 6.7-GHz and 25-GHz methanol masers in OMC-1
M. A. Voronkov, A. M. Sobolev, S. P. Ellingsen +1
The Australia Telescope Compact Array (ATCA) has been used to search for methanol maser emission at 6.7 GHz towards OMC-1. Two features peaking at 7.2 km/s and -1.1 km/s have been…
Methanol in W3(H2O) and Surrounding Regions
E. C. Sutton, A. M. Sobolev, S. V. Salii +3
We present the results of an interferometric study of 38 millimeter-wave lines of CH3OH in the region around the water maser source W3(H2O) and a region extending about 30" to the…