Polarization Properties of Astrophysical Masers

Polarization Properties of Astrophysical Masers

<p>Observed interstellar OH and H<sub>2</sub>O maser lines at 18 cm and 1.35 cm exhibit unusual polarization properties. The OH emitters with the highest brightness temperatures, usually associated with H II regions, almost always show a high degree of circular polarization. The...

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Bibliographic Details
Main Author: Kwan, John Ying-Kuen
Format: Others
Published: 1973
Online Access:https://thesis.library.caltech.edu/10392/1/Kwan_JYK_1973.pdf
Kwan, John Ying-Kuen (1973) Polarization Properties of Astrophysical Masers. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/906J-2N21. https://resolver.caltech.edu/CaltechTHESIS:08252017-145131867 <https://resolver.caltech.edu/CaltechTHESIS:08252017-145131867>

Internet

https://thesis.library.caltech.edu/10392/1/Kwan_JYK_1973.pdf
Kwan, John Ying-Kuen (1973) Polarization Properties of Astrophysical Masers. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/906J-2N21. https://resolver.caltech.edu/CaltechTHESIS:08252017-145131867 <https://resolver.caltech.edu/CaltechTHESIS:08252017-145131867>

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