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A Radiative Pumping Scheme for OH and H sub(2)O Masers in Massive Star Forming Regions
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A Radiative Pumping Scheme for OH and H sub(2)O Masers in Massive Star Forming Regions
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Journal Article
A Radiative Pumping Scheme for OH and H sub(2)O Masers in Massive Star Forming Regions
2007
Overview
Interstellar H sub(2)O and OH masers associated with massive star-forming regions can be classified into three morphological types: isolated H sub(2)O masers; isolated OH masers; and spatially overlapping OH/H sub(2)O maser groups. In a large sample of star-forming regions the total number of maser groups of each type is approximately equal. In order to account for these statistics we propose a pumping scheme based on a broadband radiative pump which produces inverted populations of both OH and H sub(2)O masers by a process involving predissociation and dissociation of H sub(2)O. This scheme overcomes some drawbacks of earlier radiative pumping models, and may account for the association of OH and H sub(2)O masers in massive star forming regions.
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