Sizes of Masing Parts of Massive Star Forming Regions

It is shown that the images, line profiles, and time evolution of different interstellar masing transitions can be explained by the hypothesis that the population inversions giving birth to masers take place in turbulent regions with extents that are orders of magnitude greater than the sizes of the...

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Bibliographic Details
Date:	2012
Main Authors:	Sobolev, A. M., Sutton, E. C., Watson, W. D., Ostrovskii, A. B., Shelemei, O. V.
Format:	Article
Language:	Russian
Published:	Видавничий дім «Академперіодика» 2012
Online Access:	http://rpra-journal.org.ua/index.php/ra/article/view/550
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Journal Title:	Radio physics and radio astronomy

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Radio physics and radio astronomy

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