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Maser Theory: Old Problems and New Insights
Published online by Cambridge University Press: 16 July 2018
Abstract
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Maser theory continues to be driven by advances in observational techniques. Here, I consider the responses to VLBI with space-Earth baselines and cross-correlation spectroscopy (a re-consideration of coherence properties), routine observation in full-Stokes polarization (a re-casting of the polarization transfer equations), and long-term variability monitoring (3-D modelling of irregular domains).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 7 - 12
- Copyright
- Copyright © International Astronomical Union 2018
References
Green, J. A., Gray, M. D., Robishaw, T., Caswell, J. A. & McClure-Griffiths, N. M. 2014 MNRAS, 440, 2988Google Scholar
Kobayashi, H., Shimoikura, T., Omodaka, T., & Diamond, P. J. 2000, in: Hirabayashi, H., Edwards, P. G. & Murphy, D. W. (eds.), Astrophysical Phenomena Revealed by Space VLBI (Institute of Space and Astronautical Science), p. 109–112Google Scholar
Landi Degl'Innocenti, E. 1988, in: Kalkofen, W. (ed.), Numerical Radiative Transfer (Cambridge, CUP), p. 265Google Scholar
Slysh, V. I. 2003, in: Zensus, J. A., Cohen, M. H. & Ros, E. (eds.), Radio Astronomy at the Fringe (ASP Conference Series, Vol. 300), p. 239Google Scholar
Zienkiewicz, O. & Taylor, R. 2000, The Finite Element Method: The basis (Oxford: Butterworth-Heinemann)Google Scholar
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