Polarization and Extent of Maser Emission from Late-Type Stars: Support for a Plasma Turbulence Model of Maser Production-Reference-Cited by-同舟云学术

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Polarization and Extent of Maser Emission from Late-Type Stars: Support for a Plasma Turbulence Model of Maser Production

Published:2001-01-20 Issue:1 Volume:547 Page:L57-L59
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Palen Stacy

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference15 articles.

1. The unusual OH envelope of U Orionis

2. U Orionis: the evolution and proper motion of the OH maser envelope

3. OH maser emission in the circumstellar envelopes of U Herculis, R Cassiopeiae and W Hydrae

4. The flare in the U Orionis OH maser

5. On the Structure of Hydroxyl Maser Sources

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. First polarimetric images of NML Cyg at 1612 and 1665 MHz;Monthly Notices of the Royal Astronomical Society;2004-02

2. Atmospheres of AGB Stars;Astronomy and Astrophysics Library;2004

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