SiO maser movies

We show how the intensity and spatial distribution of silicon monoxide masers varies with time according to the parameters of a current model. The variation of the masers at 43 GHz in the v=1 vibrational state is presented as an animation. Where possible, comparisons are drawn with a similar animati...

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Bibliographic Details
Published in:New astronomy 2000, Vol.5 (3), p.155-162
Main Authors: Gray, M.D., Humphreys, E.M.L.
Format: Article
Language:English
Subjects:
Circumstellar matter
Masers
Radio lines: stars
Stars: AGB and post-AGB
Stars: individual: TX Cam
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Summary:We show how the intensity and spatial distribution of silicon monoxide masers varies with time according to the parameters of a current model. The variation of the masers at 43 GHz in the v=1 vibrational state is presented as an animation. Where possible, comparisons are drawn with a similar animation of the real Mira variable TX Cameleopardalis.
ISSN:1384-1076
1384-1092
DOI:10.1016/S1384-1076(00)00020-8