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STUDY OF THE EMISSION PROPERTIES OF CLASS II METHANOL MASER LINES

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Parameters of the dependence between the intensities of the 51-60A+ (6.7 GHz) and 20-3−1E methanol maser lines are found: (logS6.7=0.8×logS12.2+0.8). In some maser condensations the ratio of the intensities of these lines differs significantly from this dependence. The interpretation was made that in these condensations an unknown factor acts to give additional amplification of the 51-60A+ (6.7 GHz) line.
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Keywords: Methanol masers

Document Type: Research Article

Affiliations: Astro Space Center of the Lebedev Physical Institute, Russian Academy of Sciences, Profsoyuznaya Str. 84/32, Moscow 117997, Russia

Publication date: 2002-01-01

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